The galaxy appears to be an elliptical type, exhibiting a largely featureless, smooth morphology. It presents a roughly circular shape, lacking any prominent spiral arms or a well-defined disk. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in luminosity outwards.

The color profile shows a redder core region which transitions into a slightly bluer halo. This color gradient may indicate an older stellar population dominating the central region, with a younger, more metal-poor population distributed in the outer regions. There is no indication of active star formation regions or significant dust lanes. The absence of any noticeable distortions or tidal features suggest the galaxy has not undergone a recent major merger event.
