The galaxy appears to be a relatively smooth, elliptical-like structure, with a concentrated central bulge. The light distribution suggests a fairly round morphology. There is an indication of interaction, perhaps a minor tidal disturbance or merging event with a smaller companion galaxy. This is indicated by asymmetry in the galaxy's light profile and a separate clump of luminosity on one side of the central concentration. The color is relatively uniform across the galaxy, suggesting an older stellar population and reduced recent star formation activity. It appears to be a fairly massive galaxy.
