The galaxy appears as a single, relatively smooth object with a concentrated central region. It exhibits a generally elliptical morphology, showing a relatively round shape with a very slight elongation. The color gradient transitions from a bright, yellowish core to a greenish outer halo. The central region is predominantly yellow, which may indicate an older stellar population with a lower rate of ongoing star formation. The outer region displays a faint, diffuse greenish hue, potentially associated with younger stars. There is very little evidence of spiral arm structure or significant dust lanes. The general smoothness of the light distribution is typical of an elliptical or lenticular galaxy. There are no distinct features suggesting a major interaction or merging event in the recent past. However, there seems to be some subtle disturbance of the outer halo.
