The galaxy presents a generally smooth and elliptical morphology. The core exhibits a bright, concentrated luminosity, suggesting a dense stellar population. The light transitions from a warm orange-yellow hue at the core to a cooler blue at the outer edges. There are very minor indications of a disk-like structure, but the galaxy appears dominated by its spheroidal component. Minimal distortion is apparent, with no strong evidence of ongoing mergers or tidal interactions. The color gradient suggests a gradient in stellar populations, potentially indicating older stars concentrated in the core and younger, bluer stars in the outer regions. Overall, the galaxy appears to be a relatively quiescent, well-established elliptical galaxy, possibly exhibiting a moderate level of star formation, concentrated mainly on the outer regions.
