The galaxy presents as a moderately bright object with a smooth, somewhat elongated morphology. Its central region is more concentrated and luminous, exhibiting a bright, almost unresolved core. Moving outward from the center, the galaxy displays a diffuse halo of fainter light. There appears to be a subtle extension or tidal feature emanating from the galaxy, suggesting possible gravitational interaction with another galaxy or recent merger activity.

Coloration appears generally bluish, hinting at the presence of younger stellar populations or ongoing star formation. The relative lack of distinct spiral arms or dust lanes lends credence to the notion of this being an elliptical or lenticular galaxy, although some irregular features are apparent, which could be from the aforementioned tidal disruption. Overall, the galaxy's morphology suggests it is in a state of dynamic evolution.
