This galaxy presents a somewhat flattened, elliptical morphology. The central bulge region exhibits a concentrated, yellowish-white glow, suggesting a population of older stars. A faint, bluer disk component is discernible surrounding the bulge, indicative of ongoing star formation. The disk appears relatively smooth, lacking prominent spiral arm structures. The galaxy doesn't seem to display any signs of major mergers, although there might be evidence of a minor disturbance on one side, potentially hinting at an interaction or a past merger event. Overall, the galaxy seems to be a transition type, between a pure elliptical and a spiral galaxy, exhibiting characteristics of both.
