The galaxy presents a primarily smooth morphology, suggesting an elliptical classification, but with possible features of a disk galaxy. It exhibits a pronounced elongation, with a cigar-like shape. There's no clear evidence of recent major merger activity or tidal disturbances, though minor disturbances cannot be ruled out. The color profile suggests the presence of older stellar populations, and a moderate overall star formation rate, though activity is relatively low. The galaxy core appears to be relatively bright. The structure has a concentrated central region, and a gradual decrease in luminosity towards the outer edges.
