The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light profile. Its color suggests a population of older stars, with a noticeable red/yellow hue in the core region which fades to more green/blue at the edges. There are no apparent spiral arms or significant dust lanes visible. The galaxy exhibits a somewhat rounded shape, though not perfectly circular. There is no strong evidence of ongoing major merger activity, although a minor disturbance cannot be entirely ruled out due to the faint outer regions. The overall appearance suggests a relatively evolved system with a moderate stellar mass and moderate levels of star formation.
