The galaxy presents as a mostly smooth, elongated structure. Its overall shape resembles a cigar or spindle when viewed from our perspective. The central region exhibits a concentrated brightness, likely indicative of a dense stellar population or potentially an active galactic nucleus, although there is no evidence of any. There's a color gradient across the galaxy, with a tendency towards yellower hues in the central bulge region, suggesting older stellar populations, and bluer tints toward the outer edges, hinting at the presence of younger, hotter stars and possibly some on-going star formation. There are no obvious spiral arm structures, and the light is smoothly distributed throughout the galactic body, which indicates that it may be an elliptical galaxy. There are subtle signs of a potential disturbance within the galaxy's structure, though it is not overwhelmingly visible.