The galaxy appears as a moderately luminous object with a generally smooth morphology. The light profile seems relatively concentrated, suggesting an elliptical or lenticular type. There appears to be some interaction with nearby systems. Possible distortion in its shape could be related to a close encounter or merging event with other galaxies in the group. There is a dominant central component, and a fainter, more diffuse halo surrounding it. The color appears to be somewhat reddish, suggesting an older stellar population and potentially a low star formation rate. The galaxy's overall structure does not present a well-defined spiral arm structure or a prominent disk.
