The galaxy presents as a relatively compact object with a flattened, elliptical morphology. The light distribution suggests a smooth profile without prominent spiral arms or a distinct bulge. The galaxy's color index, estimated from the image, indicates a presence of both older stellar populations, suggested by the redder hues, and potentially some younger, star-forming regions showing bluer tones. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers, though there could be some minor irregularities in the outer regions of the galaxy. The central region is more concentrated and luminous than the outer regions. Its orientation presents it almost edge-on from our point of view.
