The galaxy presents as a roughly elliptical, unresolved object. Its central region exhibits a high surface brightness, appearing nearly uniform and concentrated. The color of this central bulge is predominantly yellow-white, suggesting an older stellar population. Moving outward, the luminosity gradually decreases towards the galaxy's edges. The outer regions display a slightly bluer hue compared to the core, indicating the presence of some younger stars, though not prominently. There is no obvious spiral arm structure or distinct disk visible. The overall texture of the galaxy appears smooth, with only subtle irregularities in the light distribution. There is no evidence of tidal tails or significant distortions that would suggest a recent major merger event, although subtle disturbances cannot be ruled out.
