The galaxy presents a generally smooth morphology, with a high degree of central concentration. The overall shape appears elliptical. There is a slight elongation, more tending towards a rounded, yet cigar-shaped form rather than a perfectly circular appearance.

Color gradients suggest a stellar population that is relatively old. The core region exhibits a yellowish-orange hue, indicative of a population dominated by older stars. Fainter, bluer regions are observed extending outward from the central bulge.

There is no evidence of any significant disturbances or interactions with other galaxies, nor any indications of spiral arm structures, confirming a relatively undisturbed evolutionary state. 
