This galaxy exhibits a moderately elliptical morphology. The core region presents a concentrated, bright, and smooth appearance, possibly indicative of an older stellar population. Moving outward from the core, a faint, disk-like structure is observed, though with limited discernible features. The color distribution suggests a mixture of stellar populations; the central region appears more yellow/white, potentially indicating older stars, while the faint disk shows subtle bluish/greenish hues, which might suggest the presence of some younger, hotter stars or ongoing star formation, though not very prominent. The overall structure seems relatively undisturbed, with no strong indications of major mergers or tidal disruptions. Some minor asymmetry or subtle warping cannot be entirely ruled out, based on the slightly irregular shape.
