The galaxy presents as an elliptical morphology. The primary structure consists of a relatively smooth, centrally concentrated bulge region exhibiting a yellowish-white hue. This bulge appears to be the dominant feature, contributing significantly to the overall luminosity. 

Surrounding the bulge is a fainter, more diffuse halo or disk-like structure. This outer region displays a slightly bluer tint compared to the bulge, potentially indicating the presence of a younger stellar population. The overall shape seems to be rounded, with only a slight deviation towards an elongated form. There are no distinct spiral arms or prominent dust lanes visible, lending further credence to its classification as an elliptical galaxy.

There is no evidence of significant ongoing mergers or major disturbances to the overall structure. The galaxy appears relatively isolated and undisturbed within its environment, suggesting it is currently in a state of relative equilibrium.
