The galaxy exhibits a generally smooth morphology, with a noticeable lack of distinct spiral arms or prominent dust lanes. The light distribution is concentrated towards the center, suggesting a significant central bulge component. The shape appears to be somewhat elliptical, deviating slightly from a perfect circle, but not drastically elongated. There's a subtle color gradient, with the central regions appearing more yellowish-white, potentially indicating an older stellar population. The outer regions have a faint blue tinge, which could be attributed to the presence of younger, hotter stars, though the overall star formation rate seems to be comparatively low. There is no visual evidence of on-going major mergers, although the slight asymmetry could be indicative of minor tidal interactions or recent accretion events, even though this galaxy is mostly undisturbed. The overall impression is that of a relatively quiescent galaxy, likely an early-type spiral or lenticular galaxy transitioning towards a more passive state.
