The galaxy presents as a smooth, elliptical morphology. There's a concentrated central bulge, with the light intensity gradually decreasing towards the edges, giving it a diffuse halo. The overall shape is elongated, appearing cigar-shaped, rather than perfectly spherical. There are no apparent spiral arms, dust lanes, or signs of ongoing major mergers or tidal disturbances. The color profile indicates a population of older stars, predominantly emitting in the redder wavelengths, with a possible slightly bluer core.