The observed galaxy presents a moderately bright, elliptical morphology. It exhibits a notable central bulge, characterized by a high concentration of light, suggesting a significant population of older stars. The galaxy's overall color appears relatively blue, implying the presence of some ongoing star formation activity. Subtle disturbances are visible in the outer regions, potentially indicative of minor gravitational interactions or past merger events. There also seems to be artifacts surrounding the image. However, the core of the galaxy seems to be bright. Overall, the galaxy appears to be a somewhat compact system.
