The galaxy presents as a relatively compact object. The central region exhibits a moderate concentration of light. The overall color profile suggests a stellar population with a mix of ages, with some evidence of older, redder stars alongside younger, bluer stars. The morphology appears somewhat disturbed, possibly indicating interactions or recent mergers. There is evidence of faint tidal features and light disruption in the overall shape of the galaxy. There appears to be a lack of distinct spiral arm structure. The light emitted from this galaxy suggests a moderate mass. There is some indication of star formation activity. 
