The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The color profile suggests an older stellar population, exhibiting a yellowish hue, particularly pronounced in the core. There is a subtle color gradient, with the outer regions appearing slightly bluer than the central region, potentially indicating some ongoing, albeit limited, star formation in the galactic outskirts. The galaxy appears largely undisturbed, showing no signs of significant tidal interactions or major morphological disruptions. The overall shape is nearly circular, indicating a low degree of ellipticity. Any disc-like structure is subdued, if present at all. The galaxy lacks prominent dust lanes or spiral arm structures.
