The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears a yellowish hue, suggesting a population of older stars. The galaxy appears more elongated and slightly cigar shaped, with a high degree of central concentration. There is little to no evidence of spiral arms or significant dust lanes. The overall color is redder, consistent with a more evolved stellar population and lower levels of on-going star formation. There are no obvious signs of tidal disturbances or interactions with other galaxies. The galaxy exhibits a smooth, undisturbed morphology.
