The galaxy presents a generally smooth, elliptical morphology. The light profile appears highly concentrated towards the center, with a relatively rapid decline in surface brightness moving outwards. It exhibits a dominant spheroid component and little evidence of spiral arm structure or a prominent disk. The galaxy's color appears relatively uniform, with a reddish-orange hue, suggesting an older stellar population and a lack of significant ongoing star formation. There is no noticeable dust lane structure or signs of tidal disturbance or interaction with another galaxy. It seems to be a fairly isolated and evolved system.
