The galaxy appears to be an elliptical galaxy with a smooth, somewhat elongated morphology. The core of the galaxy exhibits a concentrated, bright yellow-white light, suggestive of an older stellar population. Moving outward from the core, the light gradually diminishes. The galaxy's color profile is fairly uniform, with only slight hints of bluer hues in the outer edges of the disk, suggestive of some younger star formation regions. The galaxy does not display any obvious spiral arm structures or significant dust lanes, appearing largely featureless. There is no indication of ongoing major merger events or significant tidal disturbances.
