The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. A high degree of central concentration is noticeable with a bright, slightly off-center core. The light profile appears to decrease gradually from the core outwards, lacking any distinct spiral arm structures or prominent dust lanes. The overall color is yellowish, suggesting a stellar population dominated by older, redder stars with minimal ongoing star formation. There are no prominent tidal features or distortions visible, indicating a relative state of equilibrium and lack of recent major merger events. A slight color variation exists, a redder concentration on the right side of the galaxy, perhaps due to a distinct cluster of older stars or a region of dust obscuration. Overall, this galaxy seems consistent with a passively evolving elliptical galaxy.
