The galaxy presents as a somewhat elliptical structure, exhibiting a concentrated central bulge that graduates into a diffuse, extended halo. The color profile suggests a dominant older stellar population, with a yellowish-red hue more pronounced towards the core. There is minimal evidence of distinct spiral arm structures or significant dust lanes. The smooth appearance indicates a relatively quiescent system, potentially undergoing low levels of star formation. The elongation of the galaxy indicates a possible oblate spheroidal shape, with the major axis significantly longer than the minor axis. Subtle irregularities in the outer regions may suggest past minor interactions or internal disturbances, however, the system seems to be relatively isolated, with no clear signs of a major merger event in progress.
