The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears to be a more yellow hue, possibly indicating a population of older stars. Surrounding this central region is a fainter, more diffuse disk component. A hint of spiral structure is suggested by subtle color variations. The galaxy doesn't show obvious signs of major mergers or significant tidal disturbances, but some asymmetry or a faint plume might indicate minor interactions. Based on the color profile, some star formation appears to be occurring, but most of the light is coming from relatively older stellar populations. Overall, the galaxy is a transition type object, between pure elliptical and spiral.
