The galaxy presents as a system with a central bulge and a discernible disk component. The bulge appears yellowish-white, suggesting a population of older stars. The disk component appears tilted, with the central region appearing more luminous. The overall shape is elongated, neither perfectly spherical nor highly flattened. There is a slight irregularity in the disk's morphology, hinting at possible tidal disturbances or past interactions. The galaxy's color profile indicates a concentration of older stellar populations and limited ongoing star formation. Based on its morphology, the galaxy is likely a disk galaxy undergoing slow evolution.
