The galaxy presents a primarily elliptical morphology, appearing mostly smooth in texture. A prominent central bulge dominates the galaxy's structure, exhibiting a concentrated luminosity that gradually diminishes towards the outer regions. The light distribution suggests a fairly uniform stellar population, but the slightly oblate shape and subtle color variations imply some degree of internal structure or ongoing processes. The color profile indicates a prevalence of older stars with a redder hue in the central regions, transitioning to slightly bluer shades in the outer edges which suggests more recent star formation may have occurred in those areas. There are no clearly defined spiral arms or distinct features to indicate significant ongoing mergers or tidal interactions. The galaxy appears relatively isolated and undisturbed, characteristic of a mature, evolving system.
