The galaxy presents as a generally smooth, centrally concentrated object with an elliptical morphology. The central region exhibits a bright, yellowish-white core, suggesting a significant population of older stars. The light gradually diminishes in intensity towards the outer regions. The overall shape is elongated, though not exceptionally so, appearing somewhat "in-between" round and cigar-shaped. There's no readily apparent evidence of spiral arms or a distinct disk structure. The galaxy doesn't obviously show signs of significant tidal distortions or ongoing major mergers, although some minor disturbance cannot be ruled out.
