This galaxy exhibits characteristics of an early-type spiral or lenticular galaxy, appearing relatively smooth and centrally concentrated. The color gradient suggests a bulge dominated morphology with a substantial population of older stars, which manifest with yellow and redder tones towards the center, although it is not perfectly round. Faint blue hues are present on the outer edges of the galaxy, potentially indicative of some younger star formation, but likely at a low rate. There are no obvious signs of strong tidal distortions or a major merger event, though a subtle asymmetry might indicate minor interactions in its past. The light distribution is quite even without large or dominating star forming regions visible. Overall, the galaxy appears to be relatively evolved.
