The galaxy presents as an elliptical or lenticular structure, exhibiting a smooth, mostly featureless morphology. It possesses a high degree of central concentration, with luminosity gradually decreasing towards the outer edges. The galaxy appears elongated with an intermediate axis ratio, suggesting a possible transition between a rounder elliptical and a more flattened, disk-like shape. The central region is yellowish, indicative of an older stellar population likely dominated by red giant stars. Faint bluish extensions are visible at the edge of the galaxy, suggesting the presence of a younger, hotter stellar population, though the star formation rate is generally low. There is no distinct spiral arm structure or prominent dust lanes. The galaxy appears relatively isolated, with no clear signs of ongoing or recent major merger events. However, there may be minor disturbances in the outer halo.