The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its color profile suggests a redder core region surrounded by a less red halo. The galaxy appears nearly round with no obvious spiral arm structure or significant morphological distortions indicative of a major merger event. There may be some very minor disturbance present. The central region is bright and dominates the overall luminosity. The outer regions fade gradually into the background, without distinct edges, suggesting a diffuse stellar halo.
