The galaxy presents as a relatively smooth, elliptical structure with a highly concentrated central bulge. The light profile appears to decrease gradually from the center outwards, with no distinct spiral arm features visible. The galaxy exhibits a somewhat spherical shape, with minimal elongation. There is a noticeable color gradient, with the central bulge appearing more yellow-orange, potentially indicating a population of older stars. The outer regions show a bluer hue, possibly suggesting the presence of some younger stars. The galaxy does not show any obvious signs of interaction or tidal disturbances. Overall, the observed morphology suggests a relatively evolved galaxy, likely an elliptical, that does not exhibit a high rate of star formation.
