The galaxy presents as a slightly elliptical, centrally concentrated system. The core region exhibits a bright, smooth, and relatively homogeneous light distribution, suggesting a dominant population of older stars. The overall color profile leans towards the redder end of the spectrum, indicative of a stellar population that is not actively forming many new stars. The galaxy is relatively compact, with a fuzzy outer halo. There are subtle hints of faint, extended structure around the main body of the galaxy, possibly indicative of a past minor merger event or tidal interactions. The morphology is generally smooth, without prominent spiral arms or a distinct disk structure.
