The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It exhibits an elliptical appearance, although it deviates somewhat from a perfectly circular shape. A bulge component is discernible, showing a gradual decline in luminosity towards the outer regions. The color profile suggests a population of older stars, potentially indicating a relatively low star formation rate. There is also a potential companion galaxy nearby. There are no obvious signs of significant tidal disturbances or active galactic nuclei features in this image.
