The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a high degree of smoothness and concentrated light, suggesting a prominent bulge. The outer regions appear less defined, with a gradual decrease in surface brightness towards the edges. There is a suggestion of a disk structure, but the smooth appearance dominates, masking any distinct spiral arm features. The galaxy's color is a muted yellow-white, indicative of an older stellar population. There is no strong evidence of significant ongoing star formation activity based on the color distribution. No signs of major merger activity or strong tidal disturbances are immediately apparent, though subtle asymmetries cannot be ruled out due to the resolution limitations. The overall structure points toward an elliptical galaxy or a lenticular galaxy viewed at a shallow angle.
