This galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse morphology without prominent spiral arms. It appears moderately elongated, with a cigar-like shape. The central region is noticeably brighter and exhibits a reddish hue, possibly indicative of an older stellar population or significant dust extinction. Moving outwards, the galactic disk displays a bluer color, suggesting the presence of younger, hotter stars. No significant tidal disturbances or signs of a major merger event are readily apparent, though minor asymmetries or disturbances may be present within the galactic disk. Overall, this galaxy seems relatively undisturbed and shows characteristics of an evolved stellar system.