The galaxy appears as a relatively smooth, elliptical-like structure with a bright central core. The light profile increases towards the center, with a concentrated central bulge that radiates intensely. There's a diffuse halo or envelope surrounding the bulge, exhibiting a blueish hue, suggestive of a younger stellar population or ongoing star formation. The galaxy's overall shape is somewhere in between round and elongated, without any clear spiral arm features or strong signs of a major merger event disrupting its morphology. There appears to be some slight asymmetry or minor disturbances present in the outer regions, possibly indicating past interactions or minor merger events. The color gradient suggests that the core may be older and dominated by redder stars, while the outer regions contain a bluer, younger population.
