The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits a generally elliptical morphology, appearing somewhat elongated rather than perfectly circular. The light profile suggests a bulge-dominated system with a gradual falloff in brightness from the core. The central region appears yellowish-orange, implying an older stellar population. There is a subtle color gradient moving outwards from the core with the outer regions exhibiting a slightly bluer hue, indicative of the presence of some younger stars. No prominent spiral arms or distinct features are readily discernible. There may be some minor disturbances, but they are not a major characteristic of the galactic structure.
