The galaxy presents an elliptical morphology, appearing elongated with a high degree of smoothness throughout its structure. A central bulge region is clearly visible, exhibiting a bright, concentrated luminosity. The isophotes suggest a moderate ellipticity, neither perfectly spherical nor excessively flattened. There is a subtle color gradient observed moving outward from the core, with the central region displaying a yellower, and redder hue. This could indicate a population of older stars dominating the bulge and evidence of dust presence. The outer regions appear fainter and bluer, indicative of a less dense stellar population and potentially a low level of ongoing star formation. No distinct spiral arms or prominent dust lanes are visible. There does not appear to be any evidence of a major merger. Possible minor tidal features suggest the presence of a small-scale interaction.
