The galaxy appears to be a relatively compact, elliptical galaxy, possibly an early-type spiral, seen nearly face-on. The light distribution is smooth and centrally concentrated with no distinct spiral arm structure or prominent dust lanes visible. There's a smooth, diffuse halo extending outwards from the central region. The galaxy shows a yellowish-white hue, suggesting an older stellar population with fewer young, blue stars. The color gradients indicate a possible variation in metallicity or stellar populations from the center to the outer regions. There are subtle signs of asymmetry or tidal features in the outskirts, indicating it may have undergone a past or ongoing interaction. Based on the morphology, this is likely a massive galaxy with a correspondingly low specific star formation rate.
