The galaxy presents as a generally smooth, elliptical-like structure with a discernible central bulge. Its overall shape is somewhat elongated. The light distribution suggests a concentration of older stars in the core, exhibiting a yellowish hue, possibly indicating a population of evolved stars. Fainter, bluish-tinged material extends outward, potentially representing a disk component with a younger stellar population or regions of recent star formation, though such features are not distinctly resolved. There appears to be a subtle disturbance in the galaxy's symmetry; potentially the result of a minor interaction or internal dynamics, but further data is needed to determine the precise nature of this irregularity.