The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a gradual decrease in surface brightness extending outwards. There is little indication of prominent spiral arms or disk features in the available image data, suggesting an older stellar population. The galaxy exhibits a yellowish-red color, indicating a possible prevalence of older, redder stars. The overall morphology suggests a lack of significant ongoing star formation activity. There is no evidence of any major ongoing mergers or tidal disturbances, which is consistent with the generally smooth appearance. The galaxy's shape is nearly round, deviating little from spherical symmetry.
