The galaxy presents as a moderately bright, relatively small object with a somewhat elliptical morphology. The light distribution appears to be concentrated towards the center, exhibiting a distinct, bright central bulge. The surrounding disk is not well-defined.

There is evidence of possible disturbances, with a hint of asymmetry and what could be tidal features or minor interactions, potentially indicative of an ongoing or past merger event. Overall, the galaxy appears relatively smooth and well-defined, with features suggestive of a galaxy undergoing or having undergone a disturbance. The color indices suggest the presence of intermediate-age stellar populations.
