The galaxy presents a roughly elliptical morphology, with a bright, concentrated central bulge exhibiting a primarily bluish color. The core region appears largely featureless, indicating a likely absence of significant dust lanes or active star-forming regions immediately surrounding the galactic nucleus.

Extending outward from the central bulge, a fainter, diffuse disk is observed. The color transitions from blue in the center to more greenish and reddish tones towards the outer edges of the disk. These color variations suggest a gradient in stellar populations, with potentially older, redder stars dominating the outer regions, and younger, bluer stars concentrated towards the core.

There is a subtle suggestion of minor disturbances in the outer disk morphology, possibly indicating past interactions or mergers. This is supported by a slight lopsidedness in the distribution of the outer disk material.

Overall, the galaxy exhibits characteristics of an early-type spiral or lenticular galaxy, where disk features are present but less pronounced than in late-type spiral galaxies, with a relatively large and smooth central bulge.
