The galaxy appears to be a relatively smooth, elliptical type. It exhibits a cigar-like shape, with an elongated profile. There is a concentration of light toward the center, which fades gradually toward the edges. The galaxy shows a predominantly reddish hue, potentially indicating an older stellar population, with a hint of yellow. No distinct spiral arms or significant dust lanes are visible within the galaxy's structure. There are no signs of major disturbances or ongoing merging activity. The galaxy appears to be relatively isolated and undisturbed.