The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless appearance. The central region is brighter and displays a yellowish hue, likely indicative of an older stellar population. Fainter, bluer light extends from the core, which suggests a small amount of recent or ongoing star formation. The overall color profile suggests a system with a dominant population of older stars, with only slight pockets of blue from newly formed stars. The shape of the galaxy appears roughly rounded. There are no apparent tidal tails, obvious signs of galactic interactions, or significant dust lanes visible. The galaxy shows no evidence of major morphological disturbances.
