The galaxy presents a slightly elongated, elliptical morphology, appearing more rounded than cigar-shaped. There's a bright, concentrated central bulge that transitions outward to a more diffuse disk or halo. The color profile suggests a predominantly older stellar population, exhibiting a yellowish to orange hue in the central region. The outer regions show a bluer tint, possibly indicating some ongoing, though relatively low, star formation. Evident disturbances and irregular features are noticeable, indicating an ongoing or recent interaction. These features are not extreme, suggesting minor disturbances more so than a major merger. There may be some disk-like structure, although it is difficult to tell because of the smoothness of the image. 
