The galaxy presents a centrally concentrated luminosity profile, suggesting a relatively smooth morphology. The central region exhibits a yellowish-white hue, potentially indicative of an older stellar population dominating the core. Moving outwards, a subtle transition to a bluer colour suggests the presence of a younger stellar population in the outer regions. The overall shape appears to be close to elliptical but is neither perfectly round nor elongated. There is no obvious visual evidence of spiral arm structures or a prominent disk. The absence of strong tidal features or significant morphological distortions suggests that the galaxy has not undergone a major merger recently, although a minor disturbance cannot be ruled out. The galaxy appears relatively isolated and no companion galaxies appear close by, meaning it is not undergoing major interactions. 
