The galaxy presents as a singular, centrally concentrated object. The light profile exhibits a generally smooth appearance, with a significant fraction of the galaxy's light concentrated in a relatively compact region. The shape is predominantly intermediate in roundness, trending towards an elongated, cigar-like morphology. There is a faint suggestion of asymmetry in the outer regions, with potential indication of minor tidal disturbances, though the structure is not clearly indicative of an ongoing major merger event. The overall color suggests the presence of an older stellar population.
