The galaxy presents a generally smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The light distribution indicates a high degree of central concentration, with brightness decreasing gradually towards the outer regions. The core appears to be relatively small, possibly indicating it hosts an older population of stars. The overall color is somewhat uniform and leans towards the redder end of the spectrum, suggesting the presence of older stars. There is very subtle evidence of some minor disturbances in the outer regions, potentially from an unresolvable interaction with a smaller galaxy or past minor mergers. 
