The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth, featureless morphology. It presents a concentrated central bulge that graduates outward into a more diffuse halo. The light distribution indicates older stellar populations, with a yellowish-red hue dominating the galaxy's overall color. There is very little visual evidence of ongoing star formation, with a lack of distinct blue regions associated with younger, hotter stars. The galaxy appears relatively undisturbed, with no major signs of tidal tails or significant morphological distortions indicative of recent mergers or interactions.
