The galaxy presents as a moderately inclined, disk-dominated system with an approximate red shift of 0.12. Its morphology is predominantly characterized by a smooth, elongated structure, indicative of a late-type galaxy. There is no bar structure visible. The central region exhibits a slightly more concentrated luminosity profile, transitioning to fainter, more diffuse outer regions. The disk appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. The color gradient from the central bulge outwards suggests a possible decline in stellar population age and/or dust content moving away from the center. The observed light likely originates from a combination of older stellar populations within the bulge and younger stars within the disk.
