The galaxy presents as a relatively compact object with a generally smooth morphology. The color profile suggests a dominant older stellar population, with the core showing a subtle blueish tint. The galaxy exhibits a moderate level of roundness. There is little to no evidence of spiral arm structure or significant dust lanes. The overall impression is that of an early-type galaxy, likely an elliptical or lenticular. The image shows no obvious signs of ongoing major merger activity, but a subtle asymmetry suggests the possibility of a minor interaction or recent accretion event.
