The galaxy presents as a generally smooth, centrally concentrated light distribution, appearing elliptical in shape. There is some indication of a possible tidal interaction or minor disturbance on the outskirts of the galaxy, visible as a slight asymmetry in the outer halo. The galaxy's central region exhibits a yellow-red hue, potentially indicative of an older stellar population and/or significant dust obscuration. No distinct spiral arm structures or prominent star-forming regions are readily apparent, suggesting it is a relatively quiescent galaxy in terms of current star formation.
