The galaxy presents as a generally smooth object with an elliptical morphology. There is minimal evidence of spiral arm structure or significant disk features. The light distribution is concentrated towards the center, indicating a prominent bulge. The galaxy's color is slightly yellow, suggesting an older stellar population and a relatively low ongoing star formation rate. There are indications of minor disturbances within the galaxy, possibly suggesting an interaction with a smaller galaxy or a past merger event. The majority of the light appears to be evenly distributed, with a smooth transition in color from the center to the outer edges.
