The galaxy presents as a relatively compact and centrally concentrated object. Its overall morphology appears elliptical or lenticular. A smooth light profile is apparent, indicative of a mostly older stellar population. A slight blue tint may indicate a small population of younger stars, but the dominant color is redder, which would suggest a reduced rate of star formation. There are no obvious spiral arms or a prominent disk component visible. Faint tidal features cannot be ruled out, though there is no clear evidence of a recent major merger. It could be undergoing a minor merger event. The galaxy appears to be located at moderate distance from Earth, considering it is not as clear as closer galaxies are.
