The galaxy presents as a moderately luminous, elongated structure with a smooth appearance. The central bulge exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population and minimal ongoing star formation in the nucleus. The outer regions of the galaxy display a bluer tint, possibly indicating the presence of younger stars or regions of recent, though subdued, star formation. The galaxy's overall shape is significantly elongated, appearing cigar-shaped. There is no clear evidence of spiral arms or a distinct disk structure, which combined with the color profile, is suggestive of an early-type galaxy, potentially an elliptical or lenticular galaxy. No significant morphological disturbances or tidal features are apparent, suggesting a relatively undisturbed evolutionary history and lack of recent major mergers, though some minor disturbances cannot be ruled out.
