The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, relatively featureless morphology. It appears elongated, with a distinct major axis. The light profile suggests a centrally concentrated bulge, indicated by the brighter, yellowish hue in the central region, with light gradually diminishing towards the outer edges. There is a very faint hint of what could be a disk component, based on a slight flattening of the galaxy shape. Overall, the galaxy appears to be relatively isolated, with no apparent major merger events or significant tidal disturbances.
