The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, grading into a less defined, extended halo. The core region displays a yellowish-white hue, potentially indicative of an older stellar population. Moving outward from the core, a subtle transition to bluer colors is observable, suggesting the presence of younger stars.

The overall shape is elongated, with an approximate cigar-shaped morphology. There are no obvious signs of strong tidal disturbances, major mergers or interactions with other galaxies. The galaxy does not appear to have a prominent disk structure. It is a quiescent system, exhibiting a low star-formation rate. The galaxy exhibits a significant amount of mass, within the expected range for galaxies of similar morphology.
