The galaxy presents an overall elliptical morphology, appearing largely smooth and relatively featureless. The central region exhibits a concentrated, bright core, suggesting a high stellar density and potentially the presence of an active galactic nucleus. The light distribution transitions smoothly from the core outwards, decreasing in intensity towards the edges of the galaxy, without any prominent spiral arm structures or significant dust lanes immediately apparent. The color profile suggests an older stellar population, dominated by redder wavelengths. While the overall structure is regular, there are slight hints of asymmetry in the outer regions, possibly indicative of minor tidal interactions or past mergers, though the galaxy appears to be largely undisturbed. Overall, the galaxy seems to be a relaxed system with a relatively evolved stellar population.
