The observed galaxy exhibits a generally elliptical morphology. The light distribution appears to be centrally concentrated, with a smooth, diffuse appearance towards the core. The central region displays a brighter luminosity than the outer regions.

A color gradient is apparent, with the central region exhibiting a bluer hue, transitioning to a redder color in the outer regions. This may indicate variations in stellar populations, with younger, hotter stars concentrated in the center and older, cooler stars located further out. The galaxy shows no obvious spiral arm structure or prominent dust lanes. There is no visible evidence of a major ongoing merger or significant tidal disturbances; however, there may be minor irregularities in the outer regions hinting at a past interaction. The overall appearance suggests a galaxy undergoing passive evolution, with a significant fraction of its stars already formed.
