The galaxy presents as a moderately luminous system with an overall elliptical morphology. The core region exhibits a concentrated, bright luminosity, suggesting a substantial stellar population, potentially an older bulge. The primary body of the galaxy is relatively smooth in appearance, showing little evidence of significant spiral arm structure or prominent dust lanes. There is a slight extension of the galaxy's profile, suggesting a possible tidal feature or interaction with another galaxy. A distinct, reddish region is present on the right side of the galaxy. This could indicate a region of active star formation, likely an HII region. The galaxy's overall color suggests a mix of stellar populations with both older, redder stars and younger, bluer stars present. There are signs of a slight disturbance, which could be caused by a minor merger.
