The galaxy presents as an elongated, cigar-shaped structure. The light distribution indicates a smooth overall morphology, with a concentrated central bulge appearing brighter compared to the fainter, extended disk. The color gradient suggests a higher concentration of older stellar populations in the central region, exhibiting a more reddish hue. Conversely, the disk shows a bluer color, hinting at younger, star-forming regions, though these are not distinctly visible. The lack of clear spiral arm structures or significant dust lanes points towards a relatively undisturbed system. There are hints of possible interactions as the color in one part of the galaxy indicates a disturbance. The estimated size of the galaxy indicates that it is a few kiloparsecs across. The star formation rate is relatively low.
