The galaxy presents as a diffuse, elliptical morphology. The central region exhibits a concentrated and bright core, surrounded by a more extended and fainter halo. There is minimal evidence of spiral arm structure or distinct features. The overall color appears reddish, suggesting an older stellar population and reduced ongoing star formation. Slight irregularities can be observed in the outer regions of the halo, possibly indicating interactions or minor disturbances in the galaxy's past. The smoothness of the galaxy profile implies a mostly relaxed stellar distribution.
