This galaxy presents a relatively smooth and rounded morphology. The light distribution appears centrally concentrated with a gradual decrease in surface brightness moving outwards from the core. There is a possible faint disk or extended halo surrounding the central region, although this is uncertain due to image resolution.

The galaxy displays a color gradient, appearing slightly bluer towards the outer regions and redder toward the center, perhaps indicating varying stellar populations or dust content. A faint hint of a disturbance or asymmetry is seen, however, the source of this is unknown. There may be evidence of tidal interactions, but the image quality is not sufficient to confirm if there are any clear tidal features associated with the galaxy. The galaxy is likely to be a relatively massive system, with an estimated size of approximately 5 kpc. The star formation rate is moderately low suggesting that the galaxy is not actively forming many new stars.