The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution suggests a high degree of radial symmetry. The core exhibits a yellowish-white hue, indicative of an older stellar population. Surrounding the core is a bluer, diffuse halo that extends outwards, possibly suggesting some degree of ongoing star formation, although not at a highly vigorous rate. A slight asymmetry is observed in the outer regions, potentially indicative of a minor tidal interaction or past merger event, though no significant disturbance is immediately apparent. Overall, the galaxy appears to be a well-formed system with a predominantly old stellar population and moderate mass.
