The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge, with a relatively gradual decline in luminosity extending outward. The galaxy appears to be largely devoid of prominent spiral arm structures. The primary color is a yellowish-orange hue, suggesting a population of older stars with lower rates of star formation. There is no visual evidence of any ongoing major mergers or significant tidal disturbances. A slight asymmetry in the outer regions may indicate a minor interaction or past disturbance. The galaxy's overall shape is relatively round, exhibiting minimal elongation.
