The galaxy presents as a generally smooth, elliptical-like structure. Its shape is elongated, with a length-to-width ratio suggesting a classification leaning towards a more cigar-shaped form. The central region exhibits a concentrated brightness, indicating a dense stellar population or possible active galactic nucleus. The color gradient transitions from a yellowish-white core to a reddish outer halo, which could suggest older stellar populations in the periphery. Some minor disturbances may be present, though it appears non-merging at this time. The galaxy does not show obvious spiral arms.