The galaxy presents as a primarily smooth, elliptical structure, although some slight irregularities or features within the disk cannot be fully excluded. The galaxy exhibits an elongated shape; it is not perfectly spherical but leans towards a cigar-like form. A prominent central bulge is observed, characterized by a yellowish hue, indicating an older stellar population. The outer regions of the galaxy gradually fade, displaying a bluish tint which may point to pockets of younger stars, but mostly consist of older ones. No significant signs of ongoing major mergers or tidal disturbances are readily apparent in the immediate vicinity of the galaxy. There is a hint of a very minor disturbance to its structure, and the spiral arms, if present, are tightly wound. The general morphology suggests a mature galaxy.
