The galaxy presents as a somewhat elliptical structure with a pronounced central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Surrounding the bulge is a fainter, bluish disk. There's some indication of subtle, diffuse structure within the disk region, however there is no tightly wound spiral arm structure. The galaxy appears relatively smooth, without obvious signs of ongoing major mergers or significant tidal disturbances, though there may be some minor distortions. The overall color gradient transitions from redder in the center to bluer in the outer regions, indicative of a radial change in stellar population and/or dust content. The galaxy shows a moderate axial ratio, leaning toward a more elongated, cigar-like shape.
