The galaxy presents as an elongated, cigar-shaped morphology. It exhibits a dominant central bulge with a smooth light distribution, suggesting a primarily older stellar population. The bulge displays a reddish hue, potentially indicative of a low star-formation rate and a higher concentration of red giant stars. Fainter, diffuse disk-like structures extend from the central bulge, oriented along the major axis. These regions show a slight bluer tint compared to the bulge, hinting at the presence of younger, hotter stars and possibly ongoing, albeit limited, star formation. There is no apparent dust lane or pronounced spiral arm structure visible. There appears to be no major ongoing merger events, although some minor tidal disturbances may exist. Overall, the galaxy appears to be a relatively undisturbed system with an elliptical-like morphology seen close to edge-on.
