The galaxy presents as a relatively smooth, elliptical morphology, characterized by a centrally concentrated bulge. There is a noticeable color gradient, transitioning from a yellow-orange hue in the central region to a bluer tint in the outer regions. This suggests the potential presence of a mixed stellar population, with older, redder stars dominating the bulge and a younger, bluer population contributing to the outer halo or disk. There appears to be a slight asymmetry or disturbance in the galaxy's shape, possibly indicating a past minor interaction with another galaxy or a recent merger event. There may be evidence of tidal features or faint extensions around the galaxy. The overall light distribution is diffuse, with a gradual decline in brightness from the core outwards.
