The galaxy appears as an elliptical or lenticular system, displaying a relatively smooth and concentrated light profile. Its color suggests an older stellar population, with a yellowish-orange hue dominating the core. The absence of distinct spiral arms or a prominent disk supports the smooth morphological classification. There are no obvious signs of active star formation or prominent dust lanes within the visible structure. The galaxy exhibits a moderate degree of roundness, appearing somewhat flattened but not strongly elongated. No signs of major mergers or significant tidal disturbances are readily apparent, with the galaxy exhibiting a largely undisturbed structure. The compact nature of the system suggests a high central concentration of stars, with the majority of the galaxy's light emanating from the central region.
