This galaxy exhibits a morphology characterized by a dominant, relatively smooth spheroidal component. It presents a centrally concentrated luminosity profile, with a core region displaying a yellowish hue, suggestive of an older stellar population. The overall shape approximates a rounded form. Subtle extensions of diffuse light are visible at the periphery. These faint outer regions have a bluer color than the central core, indicating the presence of a younger stellar population. There is no apparent spiral structure or evidence of significant dust lanes within the galaxy’s visible extent. No signs of ongoing major mergers or tidal disturbances are readily discernible, though a very faint irregularity to one side may indicate a minor interaction. The galaxy’s overall appearance suggests it is an early-type galaxy, likely an elliptical or lenticular galaxy, undergoing relatively low levels of star formation.
