The galaxy presents as an elliptical morphology, appearing largely featureless with a smooth light distribution and no readily apparent spiral arms or distinct structures. The central region exhibits a higher surface brightness, suggestive of a concentrated nucleus or bulge component. Moving outward from the core, the luminosity gradually diminishes.

The galaxy appears slightly elongated, with a non-circular shape, verging on a cigar-like appearance. There is no clear evidence of any ongoing major mergers or significant tidal disturbances, though a minor perturbation might not be ruled out.

Color-wise, the galaxy exhibits a general yellowish-white hue. The color indicates a relatively older stellar population and a lack of significant ongoing star formation, suggesting a passive or quiescent state. The overall impression is of a massive, evolved galaxy.
