The galaxy appears as a centrally concentrated object with a flattened, elliptical morphology. The core exhibits a yellowish-white hue, suggesting an older stellar population. Extending outward, there is a fainter, diffuse component with a more reddish tint, particularly noticeable on the periphery, potentially indicating the presence of dust or a population of older, redder stars. A subtle bluish region is also present on one side of the galaxy, possibly indicating a region of active star formation. Overall, the galaxy presents a relatively smooth appearance, with no obvious signs of strong tidal disturbances or major ongoing merger activity, although the irregularity on one side could be the result of a past interaction. The galaxy is moderately luminous, indicative of a substantial stellar mass.
