The galaxy exhibits a flattened, elongated morphology consistent with a late-type spiral or an edge-on lenticular galaxy. The central bulge appears prominent and exhibits a yellowish-white hue, suggesting an older stellar population. The disk component shows a bluer color, possibly indicative of ongoing star formation. Faint spiral arm structures may be present, but are not clearly defined. The overall appearance suggests a relatively smooth distribution of light across the galaxy with no major distortions or signs of ongoing mergers. There is some evidence of minor disturbances within the galaxy.
