The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be dominated by a bulge component, exhibiting an elliptical morphology. There is a slight elongation, suggesting a deviation from perfect circularity. The color appears generally redder, with minimal evidence of blue star formation regions. There's an absence of distinct spiral arms or prominent dust lanes. Faint, diffuse light extends beyond the bright central region, indicative of a halo or extended stellar population. No signs of major mergers or significant tidal disturbances are visible in the immediate vicinity.
