The galaxy presents a generally elongated, cigar-shaped morphology. Its overall color profile suggests a substantial population of older stars, indicated by the prominent reddish-orange hue concentrated towards the central regions. There appears to be a higher concentration of stellar density and light emission in the center, exhibiting a bright bulge. The outer regions gradually fade in intensity, showing a diffuse halo with less distinct structure. Patches of bluer light are visible, indicating some regions of ongoing star formation. The galaxy is possibly undergoing minor gravitational interaction with a nearby galaxy, or may be a relatively undisturbed galaxy. Overall, the galaxy is likely a spiral galaxy with an active star forming region. 
