The galaxy exhibits a generally smooth morphology with a suggestion of a flattened, elliptical shape. A bright, concentrated central bulge is visible, surrounded by a less luminous, diffuse halo. There is a slight elongation present, hinting at a possible disk component, though it's not clearly defined. The galaxy's color appears to be overall redder suggesting an older stellar population with a suppressed star forming rate. Evidences of merging or tidal disturbances are very minimal or nonexistent from what can be seen in the image.
