The galaxy appears to be an elliptical or lenticular type, exhibiting a relatively smooth light distribution. There is some indication of disk-like structure, but no obvious spiral arms or strong features are visible. The galaxy displays a notable color gradient, shifting from a bluer hue towards its center to a redder tone in its outer regions. The overall shape appears moderately rounded. There is some evidence of a potential minor interaction or disturbance, with one of the galaxies appearing to be more influenced by the other. This could be indicative of a past or ongoing tidal interaction. The star formation rate appears suppressed. The galaxy is estimated to be of intermediate mass.
