The galaxy exhibits a generally elliptical morphology with a smooth, centrally concentrated light profile. The core region displays a bright, yellowish hue, suggestive of an older stellar population. Moving outwards from the core, a diffuse, greenish halo is observed. The relatively smooth light distribution indicates a lack of significant spiral arm structure. There is some slight disturbance of the generally elliptical morphology, hinting at a possible recent interaction or minor merger event. The galaxy shows a moderate level of star formation activity.
