The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. It exhibits a bright, concentrated core region, suggesting a possible active galactic nucleus or a dense stellar population. The light distribution is centrally peaked, diminishing gradually towards the outer regions of the galaxy. 

There is a subtle color gradient visible, transitioning from a bluer hue in the center to more yellow-red tones in the outer regions. This color variation may indicate a difference in stellar populations, with younger, hotter stars concentrated in the central region and older, cooler stars populating the outskirts. 

A very slight asymmetry can be observed in the outer regions of the galaxy, potentially indicative of a minor interaction or disturbance. However, no distinct tidal tails or obvious signs of a major merger are apparent.
