The galaxy presents a generally smooth appearance, with a dominant central bulge or core region exhibiting a yellowish hue, suggesting an older stellar population. There's evidence of a possible disk component, though it is not sharply defined. The galaxy has a relatively high level of spheroidal symmetry, leaning towards an elliptical morphology, with a hint of deviation from being perfectly round. There's an indication of minor disturbance or interaction with a smaller object or tidal debris, suggesting the possibility of a past or ongoing merger event. Despite the generally smooth appearance, there are hints of asymmetry in the outer regions. Star formation appears to be currently at a low level.
