The galaxy presents as a flattened, elliptical morphology. Its central region exhibits a concentrated luminosity with a yellowish hue, suggesting a population of older stars. Moving outwards, the disk displays a more diffuse bluish tint, possibly indicating the presence of younger, hotter stars and ongoing star formation. The galaxy appears elongated, with a significant cigar shape. No distinct spiral arms are discernible. There are no signs of any major mergers. The light falloff from the center to the outer regions seems relatively smooth.
