The galaxy presents as a relatively smooth, elliptical-like structure. Its morphology is characterized by a centrally concentrated light profile, with a gradual decline in brightness towards the outer regions. The core exhibits a yellowish hue, suggesting an older stellar population. The outer regions display a bluer tint, potentially indicating the presence of younger stars, although star formation is estimated to be low. The galaxy's shape appears to be somewhat elongated, deviating slightly from a perfectly circular form. There are no prominent spiral arms or bar structures visible. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or mergers with other galaxies.
