The galaxy presents as a flattened elliptical or lenticular system. The central bulge exhibits a bright, yellowish-white hue, suggesting a population of older, evolved stars. Moving outward from the core, a diffuse, somewhat indistinct disk-like structure can be observed. This structure appears to be significantly less luminous than the bulge and exhibits a slight bluish tint, potentially indicating a younger stellar population. The overall form is elongated, and the outer regions appear relatively smooth, with no distinct spiral arm features discernible. There are hints of minor dust lanes or obscuration present within the outer disk, manifesting as faint, mottled patches of reduced brightness. The galaxy appears relatively isolated with no immediate signs of tidal disruption or ongoing mergers.
