The galaxy presents a morphology consistent with an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. There is a noticeable elongation to the galaxy's shape; the axial ratio suggests it is not perfectly spherical but rather somewhat cigar-shaped. The core appears bright and possibly unresolved in this image, indicating a high stellar density. A colour gradient is observable, with the central region showing a yellowish or reddish hue, potentially indicative of an older stellar population. Moving outwards from the core, the color transitions to a bluer and less saturated color, suggesting the presence of some younger stars or lower metallicity stellar populations. The lack of clearly defined spiral arms or dust lanes supports the classification as an elliptical galaxy. Faint extensions are possible, but difficult to discern in the image. The overall appearance indicates a galaxy with a considerable stellar mass and an older, evolved stellar population.