The galaxy presents as a luminous, elliptical morphology, exhibiting a concentrated central bulge. A smooth, diffuse halo surrounds the bright core, with a gradual decrease in luminosity moving outward. The object appears generally featureless, with a lack of discernible spiral arms or distinct dust lanes. The color profile indicates a redder hue in the central regions, possibly indicative of an older stellar population. Subtle variations in color are observed within the halo, suggesting some degree of stellar population heterogeneity. The galaxy exhibits a generally regular shape.
