The galaxy presents as a flattened, elliptical morphology, appearing cigar-shaped when viewed from our perspective. It exhibits a generally smooth texture. The central region shows a concentrated brightness and a yellowish-white hue, indicating an older stellar population. Fainter, bluer light appears in the outer regions of the disk, potentially indicating regions of younger stars and ongoing star formation. There appears to be no obvious central bulge, but this is difficult to determine from the viewing angle. There is no evidence of significant tidal disturbances, major mergers, or interactions with other galaxies.
