The galaxy presents a generally elliptical morphology, exhibiting a smooth and concentrated light profile. The core region is characterized by high luminosity, suggesting a significant concentration of stars. Fainter light extends outwards, exhibiting a gradual decrease in surface brightness, however the outer regions are poorly resolved. No distinct spiral arm structures or dust lanes are evident within the observed image. There is no indication of a recent major merger event or tidal interactions. The galaxy appears relatively isolated and undisturbed. The color distribution is broadly consistent with an older stellar population. The redder hues possibly indicate a higher proportion of evolved stars.
