The galaxy presents an elongated, cigar-shaped morphology. A prominent central bulge appears to be present, with the galaxy's light appearing more concentrated towards the center. The disk component exhibits a relatively smooth texture. There is a slight hint of dust lanes running along the disk, though they are not sharply defined. The galaxy's color indices suggest a substantial population of older stars, with the overall light trending towards redder wavelengths, with an absolute magnitude of -21. It may have a high mass, likely above 10^10 solar masses. The galaxy exhibits only slight disturbances suggesting it may have undergone a minor merger in the recent past. The disk appears to have a relatively low star formation rate.
