The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. Its overall shape is elongated, displaying an approximate cigar-like form. A bright, concentrated central region, likely a bulge or core, is apparent. The galaxy exhibits a color gradient, with the central region appearing more yellowish-white, possibly indicating an older stellar population. Fainter, bluer hues extending outwards from the core may signify areas of more recent, though likely subdued, star formation activity. There appears to be a lack of distinct spiral arm structures or prominent dust lanes, reinforcing the classification as a smooth galaxy with possible recent or ongoing minor disturbances. The galaxy doesn't obviously appear to be merging with another galaxy. The estimated size corresponds to approximately 4.2 kpc.
