The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, diffuse luminosity profile with a pronounced bulge dominating the overall structure. The galaxy is elongated, displaying a slight flattening. Color gradients are subtle, with a generally yellowish hue, indicative of a population of older stars and a relatively low ongoing star formation rate. No prominent dust lanes or spiral arm structures are discernible, suggesting a lack of significant cold gas and recent merger activity. A faint halo may be present but the edges are poorly defined.
