The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with a subtle elongation that suggests a deviation from perfect sphericity. A dominant central bulge is evident, displaying a warmer color, likely indicating an older stellar population. The overall color profile is redder, suggesting a lack of significant recent star formation. There are no visually discernible spiral arms or prominent dust lanes. Slight asymmetries could indicate a minor interaction or disturbance, but it's also possible that these are merely subtle irregularities in the overall structure. The overall appearance is that of a mature galaxy with a well-established stellar population.
