The galaxy presents as a relatively bright, lenticular or early-type spiral system. Its morphology is dominated by a smooth, centrally concentrated bulge. The disk component appears faint and somewhat elongated, with subtle hints of spiral structure, potentially with a central bar. The colour profile suggests the presence of a moderately old stellar population. There is evidence of an ongoing minor merger, characterized by tidal tails emanating outwards. There is a moderate level of dust extinction. Star formation appears to be happening at a low to moderate rate. Overall, this system exhibits properties consistent with an evolving galaxy.
