The galaxy presents as a system comprised of two distinct components. The primary component appears as a largely featureless, centrally concentrated spheroid, exhibiting a smooth light distribution. Its dominant color is a relatively homogenous blue hue. The secondary component displays a less regular morphology, with a non-uniform luminosity profile and hints of internal structure. This component is offset from the primary spheroid and exhibits a yellow-red color gradient, suggestive of a slightly older stellar population compared to the primary spheroid. There is potentially some evidence of tidal disturbance. The overall morphology appears to be that of a system undergoing interaction or possible merger, characterized by the distinct features in the secondary component and the smooth, spheroidal nature of the main galaxy.
