The galaxy presents a generally smooth, elliptical morphology. The primary structure exhibits a centrally concentrated bulge that appears yellowish-orange, suggesting a population of older stars. A flattened disk component is observed, oriented approximately horizontally in the image. This disk appears less prominent than the bulge, and has a bluer hue indicative of ongoing star formation. The overall shape is not perfectly circular; it has a slightly elongated, cigar-like appearance. There is no obvious evidence of a major ongoing merger or significant tidal disturbances, though subtle asymmetries within the disk could indicate minor interactions or internal processes.
