The galaxy appears as a roughly elliptical structure with a smooth, diffuse light distribution. A central bulge region, characterized by a yellowish-orange hue, dominates the core. This central region transitions smoothly into a broader, less concentrated disk. The disk appears bluer in color, particularly toward its periphery, suggesting the presence of younger stellar populations or ongoing star formation. There is no clear evidence of spiral arm structures, strong dust lanes, or significant tidal features. The overall morphology suggests an evolved galaxy, potentially an early-type spiral galaxy.
