The galaxy presents as an elliptical or lenticular type, exhibiting a predominantly smooth morphology with a bright central bulge. There is faint, but discernible disk-like structure, though it is not well-defined. The light distribution is relatively uniform, lacking strong spiral arms or prominent dust lanes. The galaxy displays a noticeable color gradient, transitioning from a bluer hue in its outer regions to a redder tint towards the center. This color variation suggests potential differences in stellar populations, with younger, bluer stars dominating the periphery and older, redder stars concentrated within the nucleus. I notice only a slight asymmetry in the galaxy's overall structure, perhaps indicative of a past minor interaction or disturbance. There is no obvious evidence of a significant, ongoing merger. Overall, the galaxy is a reasonably evolved system.
