The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, yellowish core that suggests an older stellar population. There is a subtle, elongated shape, hinting at a possible disk component, though it is not clearly defined. Evidence of any significant spiral structure is absent. A small, redder area is slightly offset from the central region. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. The overall color suggests moderate levels of star formation.
