The galaxy presents as a smooth, elliptical-like structure, with a concentrated central bulge. Its light profile appears relatively uniform, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The overall color index suggests a population of older stars, with a subtle shift towards bluer hues in the outer regions. There is no evidence of ongoing major mergers or significant tidal disturbances, but there is a hint of some possible disturbance in the outer regions of the galaxy, indicating a possibility of a minor merger or interactions. The galaxy's morphology leans towards a spheroid-dominated system.
