The galaxy presents as a moderately bright, elongated structure. It appears largely smooth in texture, with a discernible central bulge dominating the visual profile. The overall color gradient suggests a higher concentration of older stellar populations in the central region, shifting towards bluer hues further from the core, especially along the outer edges. The galaxy exhibits a notable degree of ellipticity, tending towards a cigar-like shape. No strong evidence of ongoing mergers or major disturbances is readily apparent in this image, though subtle asymmetries and potential tidal features cannot be definitively ruled out without higher resolution data.
