The galaxy presents as a somewhat elliptical, smooth structure with a concentrated central bulge. Color gradients are subtle, with a slightly bluer periphery compared to the redder core. The smooth light distribution suggests a system dominated by an older stellar population and a relative lack of significant dust lanes or star-forming regions. There is little visual evidence of spiral arms or other prominent features. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers with nearby galaxies. Small asymmetries or disturbances might be present, but are not immediately clear. The light appears fairly uniform throughout the galaxy, with no distinct knots of star formation. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy.
