The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards, lacking distinct spiral arm structures or prominent features. There is a slight elongation in shape, with the galaxy appearing somewhat cigar-shaped rather than perfectly circular. The color profile suggests a population dominated by older stars, as the light is generally redder in overall color and hue. There is little evidence of ongoing major star formation. The galaxy appears isolated, with no obvious signs of recent or ongoing mergers or tidal disturbances from interactions with neighboring galaxies. Marginal irregular structures or low-level disturbances could be apparent.
