The galaxy presents an elliptical morphology, exhibiting a smooth and featureless light distribution. The core of the galaxy is characterized by a bright, concentrated luminosity, suggesting a high stellar density. The color gradient indicates a redder hue in the central region, potentially due to an older stellar population or dust obscuration. The outer regions display a fainter, more diffuse glow, possibly reflecting a lower stellar density at the galaxy's periphery. The overall shape is elongated, but not excessively so, appearing to be between round and cigar-shaped. Evidence of minor disturbances might be present, given the slight asymmetry in the light distribution at the edges. There are also hints of a possible merger event, though further observation is needed to confirm if the observed peculiarities are indications of an ongoing or past interaction with another galaxy.
