This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated morphology. Its overall shape is slightly elongated, deviating somewhat from perfect sphericity. The core region presents a bright, yellowish-white hue, indicative of an older stellar population. The light gradually diffuses outwards from the core, transitioning into fainter, redder tones within the galaxy's outer regions. These characteristics suggest a population of older stars.

There is no visible evidence of spiral arms, prominent dust lanes, or significant star-forming regions. The smooth appearance and color gradient suggest a relatively quiescent galaxy with a low star formation rate. There is no obvious tidal distortion or other morphological irregularities suggesting that the galaxy is undergoing, or has recently undergone, a major merger event. However, there is a slight asymmetry to the galaxy's overall shape, which may indicate a minor disturbance, or a past merger event.