The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region is bright, displaying a yellowish hue that potentially indicates an older stellar population. The overall shape is approximately round, with a slight extension visible. The galaxy appears relatively isolated, without evidence of significant tidal interactions or major disturbances in its structure. A very subtle flattening is observed, deviating slightly from a perfect spherical shape. A faint, diffuse halo is discernible, gradually fading into the background sky. There is no clear indication of spiral arms or distinct dust lanes. The galaxy's color profile suggests a relatively passive system, potentially with a low star formation rate, as inferred from the lack of strong blue colors typically associated with young, hot stars.
