The galaxy presents as a moderately luminous, elongated structure. Its overall form appears relatively smooth and undisturbed, with a high degree of central concentration. The core exhibits a yellowish hue, suggesting an older stellar population. Surrounding the core is a bluer, more diffuse envelope. The lack of clearly defined spiral arms or prominent dust lanes suggests the galaxy is likely an elliptical, or possibly a lenticular, type. There is a slight indication of minor disturbance or asymmetry within the outer regions of the envelope.
