This galaxy presents as a generally smooth and centrally concentrated system. The central region exhibits a bright, yellowish-orange hue, indicative of an older stellar population likely dominating this area. The galaxy appears relatively undisturbed, though there is a slight irregularity in the outer isophotes suggesting a possible minor interaction or internal disturbance. There is a faint, somewhat diffuse blue-ish halo surrounding the core, possibly indicating areas of recent star formation at the galactic periphery. The overall structure is broadly elliptical, with a possible faint disk component or spiral arm structure. There is no obvious major merger apparent, but the slight asymmetry suggests a past or ongoing minor interaction.