The galaxy presents as a primarily smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core indicative of an older stellar population. The galaxy's outer regions display a bluer hue, suggesting the presence of some younger stars or ongoing star formation, though this activity appears subdued. The overall morphology is regular and lacks prominent features such as spiral arms or significant dust lanes, although there is some texture around the core. The color distribution suggests the presence of a red sequence stellar population. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major mergers in its immediate vicinity. Its round shape is characteristic of elliptical galaxies.
