The galaxy presents an elliptical morphology, appearing largely smooth and featureless in the observed light. Its overall color is moderately red or yellowish, suggestive of a stellar population that is primarily composed of older stars, with limited on-going star formation. The light is concentrated towards the center of the galaxy, with a gradual decline in surface brightness moving outwards, indicating a dense central bulge. The observed shape is elongated, but not extremely so. There is no strong evidence of a disk component or spiral arm structure, suggesting a classification along the elliptical sequence. Faint irregularities are visible, though may be due to limitations in resolution. Based on its visual properties, this galaxy likely has a considerable mass and a relatively low specific star formation rate.
