The galaxy presents as a relatively smooth, elliptical-like structure, though not perfectly symmetrical. It exhibits a slightly elongated, cigar-shaped morphology. A central bulge region displays a concentrated, bright yellow-white hue, indicating a population of older stars. The disk surrounding the bulge shows a color gradient, transitioning from yellow-white near the center to a more diffuse, bluish tinge at the outer edges, potentially suggesting regions of recent or ongoing star formation. There is no clear evidence of spiral arm structures or significant dust lanes. The overall appearance suggests a galaxy that is transitioning from a spiral to an elliptical morphology. Weak disturbances are possibly present, but no major mergers are apparent. The object possesses an estimated stellar mass within the range of 10^10 to 10^11 solar masses, with a relatively low star formation rate.
