The galaxy presents as a relatively compact object with a generally smooth appearance. There is a slight elongation to its form, deviating from a perfect circular shape. The galaxy exhibits a central concentration of light, suggesting the presence of a bulge component. Faint color gradients are discernible within the galaxy, with the central region appearing slightly redder compared to the outer regions, implying a potential difference in stellar populations and/or dust content. There is little evidence of distinct spiral arms or prominent star-forming regions, supporting a classification towards early-type galaxies. Faint asymmetries or minor disturbances in the outer regions may indicate past interactions or mergers, although no significant tidal tails or other signs of ongoing strong interactions are apparent.
