The galaxy presents as a somewhat diffuse, lenticular-shaped object. Its central region exhibits a notably bright, concentrated luminosity, suggestive of an active galactic nucleus or a dense stellar population. The color of the core is predominantly yellow-orange, potentially indicating a population of older stars.

Extending outward from the core, a faint, disk-like structure is discernible. The disk appears relatively smooth, lacking prominent spiral arms. The overall color of the disk is bluer compared to the core, indicating the presence of younger stars or regions of active star formation, albeit at a low rate.

There is a slight asymmetry or disturbance in the galaxy's morphology, potentially hinting at a past or ongoing interaction or merger event. A faint tidal tail or extended halo may be present but is obscured by image quality. 
