The galaxy presents an overall smooth morphology, with a slightly elongated, cigar-like shape. The central region exhibits a high concentration of light, indicating a prominent bulge component. The color profile appears relatively uniform, suggesting a lack of significant recent star formation in the galactic disk. There are no obvious spiral arm structures or dust lanes visible. There is a slight asymmetry in the outer regions, possibly indicating a minor gravitational disturbance. The red shift shows that this is a relatively distant galaxy. Overall, the galaxy is likely a massive elliptical galaxy with a large population of older stars and low rate of star formation.