The galaxy presents as a moderately luminous object with a concentrated central region and a diffuse surrounding halo. The core exhibits a yellowish hue, suggesting a population of older stars. The outer regions appear fainter and display a slightly bluer tint, which may indicate some ongoing star formation within the disk. There is no clear spiral structure evident, and the morphology appears relatively smooth and featureless. The overall shape is roughly circular, indicating a possible elliptical or lenticular classification. There is no obvious evidence of any major mergers or tidal disturbances, although subtle irregularities may indicate minor interactions. Based on the color gradient from the core to the outer regions, there is a possibility of a mixed stellar population with the core being older and the outer regions having a younger population.
