The galaxy presents as an elliptical morphology. Its light profile appears smooth and centrally concentrated, indicative of a spheroid-dominated system. The core is a bright yellow, suggesting a population of older stars, or possibly a dust component that reddens the light. The overall shape is somewhere between a perfect circle and a cigar shape. There is no clear evidence of spiral arms, dust lanes, or other distinct features typically associated with disk galaxies. The galaxy appears relatively undisturbed, with no obvious signs of major merger activity or tidal distortions. There may be minor disturbances present, but these are difficult to see given the limited resolution of the image. Based on the colors, this system appears to be relatively passive, with a suppressed star formation rate.
