The galaxy appears to be an elliptical type. Its overall shape is elongated, with a cigar-like appearance. It exhibits a smooth, featureless profile with a concentrated central bulge that transitions gradually outward. The color gradient suggests a population of older stars, with a yellowish-orange hue dominating the central region. Fainter, bluish-white tinges are visible in the outer regions, indicating the presence of some younger, hotter stars, although the overall star formation rate appears relatively low. There may be a faint tidal tail or stream extending from one end of the galaxy, suggestive of a possible past minor interaction or merger event. No obvious spiral arms or distinct dust lanes are discernible.
