The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light profile appears relatively uniform, with a gradual decrease in intensity moving outwards from the core. There is some slight elongation, possibly indicating it is between round and cigar-shaped. No distinct spiral arm structures or dust lanes are discernible. There may be a slight irregularity in the light distribution on one side of the galaxy, possibly indicating a minor interaction or disturbance. The color is generally yellow-white, consistent with an older stellar population, and likely not a high rate of star formation. The galaxy's small apparent size indicates that it is relatively distant.
