The galaxy presents a largely smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its periphery. The color profile suggests a dominant population of older stars, with a yellowish-red hue indicating reduced ongoing star formation activity. There is little evidence of prominent spiral arms or significant dust lanes. Subtle asymmetries could suggest minor gravitational interactions, but the overall structure is relatively undisturbed. The galaxy appears well-defined, with no obvious signs of a major ongoing merger event.
