The galaxy presents as a slightly elongated, lenticular-like structure, exhibiting a smooth, centrally concentrated bulge region that emits light primarily in the yellow and red wavelengths. This suggests a population dominated by older, cooler stars. The surrounding disk appears fainter with a hint of blue color, implying a younger population of hotter stars and potentially some ongoing star formation, though the rate of star formation seems relatively low. There is no clear evidence of spiral arm structures or a well-defined bar, and the overall morphology appears relatively undisturbed, suggesting a lack of recent major merger events.
