The galaxy presents a roughly elliptical morphology, although a slight deviation from perfect roundness is discernible. The light distribution appears relatively smooth across the galactic body, with a centrally concentrated brightness profile that diminishes gradually towards the edges. The core of the galaxy exhibits a bright, compact appearance. A subtle disk structure or other defining features may exist that are difficult to confirm, but there appears to be some disk-like structure.

There are no clear signs of a major ongoing merger or significant tidal disruption. It could be classified as an early-type galaxy, potentially an elliptical, owing to its observed morphology and brightness profile. It is possible that a minor disturbance might be occurring, or that it may have occurred in the past. There is some irregularity.
