The galaxy presents a generally smooth morphology with a dominant spheroid. The shape is elongated, appearing cigar-shaped, and is likely an elliptical galaxy or a lenticular galaxy viewed edge-on or at a high inclination. The central bulge exhibits a yellowish hue, potentially indicative of an older stellar population. Fainter, bluish extensions are visible along the edges, suggesting the presence of younger stars or regions of ongoing star formation within a disk component. The absence of well-defined spiral arms supports the classification as either an elliptical or a lenticular galaxy with a truncated disk. There is no evidence of major mergers or significant tidal disturbances in its immediate vicinity, although there could be signs of minor interactions.
