The galaxy presents as a flattened, elliptical structure. It has a smooth overall appearance, showing no distinct spiral arms or flocculent features. The color gradient transitions from a slightly bluer hue towards the edges to a more yellowish-red at the central region, potentially indicating a higher concentration of older stellar populations in the core. Its elongation suggests a cigar shape, with no obvious signs of ongoing major mergers or tidal disturbances, though a minor interaction cannot be ruled out. The lack of strong blue knots or HII regions supports the observation of moderate star formation activity. The galaxy's estimated size is a few kiloparsecs, classifying it as a dwarf galaxy. 
