The galaxy appears as a slightly elongated, centrally concentrated light source. Its morphology suggests a relatively smooth distribution of stars. Color gradients are subtle, showing a slightly bluer hue in the outer regions compared to a yellower center. There is no readily apparent spiral structure or distinct features such as prominent dust lanes or star-forming regions. Overall, the galaxy exhibits characteristics consistent with an elliptical or lenticular morphology, with a relatively quiescent stellar population. Subtle disturbances can be seen on the edges of the object, but appear minor.
