The galaxy presents an overall elliptical morphology, appearing elongated and somewhat cigar-shaped. There is a relatively smooth distribution of light across the galaxy's body, but with noticeable color variations. The central region exhibits a concentrated yellowish-orange hue suggesting an older stellar population, while the outer regions display a bluer tint, potentially indicative of more recent star formation activity. There is no clear indication of a spiral structure or distinct dust lanes. Faint irregularities along the periphery may suggest minor gravitational disturbances or interactions. The overall color gradient indicates a possible transition from older stars in the core to younger stars in the outer regions.
