The galaxy presents as a relatively smooth, centralized light distribution with a moderate degree of ellipticity. The core region exhibits a bright, condensed luminosity profile, appearing almost unresolved at this resolution. The outer regions display a gradual decrease in surface brightness, fading into the background sky. There's a subtle color gradient, with the central region appearing slightly bluer than the outer halo, suggesting a possible difference in stellar populations or dust content between the two regions. No distinct spiral arms or prominent dust lanes are clearly visible, indicating it may be a relatively quiescent galaxy. Based on the smooth appearance, this galaxy appears more consistent with an elliptical or lenticular classification. There is no evidence of any major mergers, and the overall morphology suggests a dynamically relaxed system.
