The galaxy presents as a fairly smooth, elliptical-like object. Its central region exhibits a concentrated, bright yellowish-orange hue, suggesting an older stellar population. Moving outward from the center, the galaxy's color gradually fades to a more diffuse yellowish tint before finally fading to a faint bluish hue. There is no immediately apparent spiral structure or distinct dust lanes, leading to the classification of the galaxy as elliptical or lenticular. There are no signs of major disturbances or ongoing mergers, however, there appears to be minor tidal disturbances visible. The overall morphology is compact, with a relatively high degree of central concentration.
