The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a bright, concentrated luminosity with a yellow-orange hue, suggesting a significant population of older stars. Moving outwards, the luminosity gradually decreases towards the edges of the galaxy. Some regions show a slight bluer tint around the edges, possibly indicating some star formation in the disk. The morphology seems regular, with no clear signs of major tidal disturbances or merging activity. Its overall shape appears rather round. The galaxy displays a significant mass and very little ongoing star formation.
