The galaxy appears to be a relatively smooth, elliptical or lenticular system. A bright, concentrated central bulge dominates the visual structure, exhibiting a yellowish-white hue, suggestive of an older stellar population. The outer regions of the galaxy show a gradual decrease in surface brightness, with a slight flattening of the disk, however the disk does not seem to be prominent. Faint blueish tinges are apparent in the surrounding regions, possibly indicating areas of more recent, albeit limited, star formation. No significant tidal features or signs of major merger activity are visible. The morphology appears relatively undisturbed, suggesting a quiescent evolutionary state.
