The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, characterized by a bright yellowish hue, suggesting a dominant population of older stars. The overall shape is largely rounded. There's a subtle extension beyond the central region, gradually fading into the background. There's no readily apparent spiral arm structure or significant dust lane obscuration, reinforcing a smooth morphology. The galaxy appears to be relatively isolated with no clear signs of major tidal disturbances or ongoing mergers. There is a possible slight disturbance/interaction happening on one side.