The galaxy presents a flattened, elliptical morphology, appearing cigar-shaped. It exhibits a relatively smooth light distribution with a concentrated central bulge. The bulge displays a yellow-white hue, suggesting an older stellar population. The outer regions, while fainter, show a subtle blue tinge, indicating the presence of younger, hotter stars and potential ongoing star formation, although this is not immediately apparent. There is no obvious spiral arm structure or significant dust lane features visible. The galaxy doesn't appear to be undergoing any major merger events.
