The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and featureless morphology. Its color profile appears relatively uniform, tending toward a yellow-orange hue, suggesting a population dominated by older stars with lower levels of on-going star formation. The light is concentrated towards the center of the galaxy and diffuses towards the outskirts. There is a possible hint of a disk structure, but the galaxy is more prominent in the vertical direction. There are no apparent signs of major mergers or significant tidal disturbances.
