The galaxy presents a generally smooth and rounded morphology. The light distribution appears concentrated towards the center, indicating a prominent bulge. There is faint evidence of spiral structure with a tight winding. The color appears to be relatively uniform across the galaxy, with a subtle shift towards redder hues in the central regions. No prominent dust lanes or active star-forming regions are readily discernible. The galaxy appears to be relatively isolated, showing no signs of major interaction or merging with other galaxies in its immediate vicinity, however there is a faint structure offset on the top right side of the center, indicating a minor disturbance of some kind. The roundness of the bulge suggests that the galaxy is likely an elliptical or an early-type spiral galaxy viewed face-on.
