The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge. The color gradient suggests a population of older stars dominating the core, exhibiting a reddish hue. Moving outward from the core, the galaxy shows a slight shift towards greenish/yellowish tones, suggesting the presence of younger stellar populations or ongoing, though minimal, star formation within the galaxy's disk, though the overall star formation rate is observed to be low. There is no noticeable spiral arm structure. The galaxy does not show signs of major tidal disturbances or merging activity, maintaining a generally undisturbed morphology. The shape of the galaxy appears roughly round, with a slight ellipticity.
