The galaxy presents as a centrally concentrated object with a largely smooth, spheroidal morphology. The core region exhibits a yellowish hue, indicating a potentially older stellar population. The outer regions show a subtle fading in intensity, with hints of a very faint disk structure extending beyond the bright central bulge. There appears to be some low-level disturbance or irregularity in the outer structure, although the galaxy's overall shape is not significantly distorted. Star formation activity appears to be relatively low. There is no evidence of a major merger event, though minor gravitational interactions cannot be ruled out. The galaxy has an estimated redshift of 0.127, placing it at a considerable distance. The estimated diameter is approximately 5 kpc.
