The galaxy presents as a slightly inclined, disk-like structure. It exhibits a smooth, diffuse morphology, lacking any pronounced spiral arms or strong knots of star formation. The central region appears brighter and more concentrated, suggesting a bulge component. The color profile indicates a bluer hue in the outer regions of the disk, potentially indicative of younger stellar populations or ongoing star formation, while the central bulge appears yellower, possibly indicating older, redder stars. The galaxy's overall shape is elongated, cigar shaped, with no signs of major disturbances or ongoing mergers. Minor irregularities may be present, warranting further investigation.
