The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated, bright core which graduates outward in intensity. There are no discernible spiral arms or prominent dust lanes visible in this image. The shape approximates a circular form, with minimal elongation observed. The color appears relatively uniform throughout, with a tendency towards redder wavelengths, typical for galaxies with older stellar populations and ongoing star formation. No indications of major mergers or tidal disturbances are immediately apparent, suggesting a dynamically relaxed system.
