The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward from the core. There is no clear evidence of spiral arm structure or a prominent disk. The galaxy has a generally rounded appearance. There are no obvious signs of recent major merger activity or tidal disturbances. The galaxy is moderately red in color, suggesting a population dominated by older stars and a relatively low current star formation rate.
