The galaxy presents a generally smooth and rounded morphology, indicative of an elliptical or S0 type. It exhibits a concentrated central bulge with a gradual decrease in luminosity toward its outer regions. There's an absence of distinct spiral arms or a well-defined disk structure. The color profile suggests an older stellar population, with a yellowish hue dominating the image. There are no obvious signs of ongoing major merger activity or significant tidal disturbances.
