The galaxy presents as a centrally concentrated object with a relatively smooth, amorphous morphology. Its overall color appears yellowish-orange, suggesting an older stellar population and a relatively low rate of ongoing star formation. The galaxy does not show a distinct spiral arm structure or prominent dust lanes. There are no apparent tidal tails or other signs of major disturbances in the immediate vicinity, although the possibility of a past or ongoing minor merger cannot be ruled out given the presence of a subtle asymmetry to the system. It is roughly circular, being slightly elongated.
