The galaxy presents as an elongated spheroid with a relatively smooth, featureless appearance. The central region displays a yellowish hue, suggesting a higher concentration of older stellar populations. Moving outwards from the center, the galaxy gradually transitions to a faint bluish tint, possibly indicating the presence of younger, hotter stars or regions of ongoing star formation. There are no clearly defined spiral arms or other distinct morphological features visible. The overall light distribution suggests the galaxy is dominated by a bulge component with a very faint or non-existent disk. Its elongated shape indicates a classification leaning towards an elliptical galaxy, although some distortion is visible, so a spiral galaxy viewed edge on is also possible, with no distinctive features visible. There are no signs of a major merger or strong tidal interactions in this image, though some minor disturbance cannot be ruled out. 
