The galaxy presents a roughly elliptical morphology, suggesting a possible classification as an elliptical or lenticular galaxy, although some disk-like features are discernable. The central region exhibits a high degree of luminosity and appears yellowish-white, indicative of an older stellar population. Moving outward from the core, the luminosity decreases. The spiral arms exhibit a more bluish hue, implying the presence of younger, hotter stars. There appears to be minor disturbances to the shape of the disk. There are no obvious signs of a major merger event. This galaxy shows strong signs of ongoing star formation. The galaxy is reasonably massive and the rate of star formation is relatively high.