The galaxy presents as a largely homogenous, elliptical structure with a concentrated central bulge. The light profile appears smooth, indicative of an older stellar population. The color gradient suggests a greater concentration of older, redder stars toward the core, transitioning to slightly bluer hues in the outer regions, possibly indicating some ongoing, albeit low, star formation in the disk or halo. The overall morphology is largely undisturbed, with no apparent signs of major tidal interactions or recent mergers. The galaxy is moderately luminous, suggesting a substantial stellar mass.
