The galaxy presents as a generally smooth, round morphology. It exhibits a notable concentration of light towards its center, indicative of a bulge. The object displays a color gradient, shifting from redder hues at the core towards yellower tones in the outer regions. There is no clear evidence of spiral arm structures or significant disk-like features. The galaxy appears relatively undisturbed, showing no signs of ongoing major mergers or tidal distortions. Its apparent size is small suggesting it is at a significant distance. Given its color and smooth profile, the galaxy is potentially an elliptical or S0 galaxy, likely composed of an older stellar population, with low star formation rate.
