The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a high stellar density. Moving outward from the core, the light profile gradually diminishes, showing no distinct spiral arm structures or prominent dust lanes. The overall color appears to be redder, suggesting a population dominated by older stars and a relatively low rate of ongoing star formation. There is no visual evidence of any major mergers or tidal disturbances in this image, and the galaxy appears largely undisturbed. The isophotes are smooth and relatively regular, with a slight elongation detectable.
