The galaxy presents an elliptical morphology with a smooth, relatively featureless light distribution. The core exhibits a bright and concentrated region, surrounded by a more diffuse halo. Color gradients suggest a possible aging stellar population, with a redder hue toward the outer regions. There is a faint disk structure, that is elongated with an estimated axis ratio of approximately 0.5 and rotated roughly 6 degrees relative to the horizontal axis. The galaxy shows no visible signs of spiral arms or significant dust lanes. There is no obvious evidence of recent major merger activity, although minor disturbances cannot be ruled out. The galaxy's estimated effective radius is small. Overall, the galaxy appears to be a relatively undisturbed early-type galaxy.
