The galaxy presents an elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. It shows a prominent bulge with a gradual decrease in luminosity outward, suggesting a well-established stellar population. The color profile transitions from a reddish hue in the core to a slightly bluer periphery, possibly indicating some ongoing star formation in the outer regions, although the overall color suggests a relatively older stellar population. No apparent spiral arms or distinct features indicative of recent mergers or significant disturbances are visible. The overall shape is somewhat elongated, deviating slightly from a perfectly circular form.
