The galaxy presents as a lenticular or possibly an elliptical type, exhibiting a smooth, centrally concentrated morphology with a noticeable bulge. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, indicative of a lack of recent star formation in this area. Moving outward from the core, the galaxy maintains a fairly uniform, though slightly bluer color profile. The galaxy appears elongated, with its shape being somewhere between a flattened disk and a cigar shape. There is no immediately visible evidence of a strong ongoing interaction or major merger events. It is a relatively isolated galaxy displaying no significant morphological disturbances or tidal features within this field of view.
