The galaxy presents a generally elliptical morphology. Its light profile appears smooth and centrally concentrated, with a gradual decrease in brightness from the core to the outer regions. The color indices suggest the presence of an older stellar population, with a dominant yellow-orange hue in the core and a slight shift towards blue in the outer regions. There's no obvious presence of spiral arms or a prominent disk.

The galaxy shows no signs of major disturbances indicative of ongoing or recent major merger events. However, there are minor asymmetries and irregularities in the outer regions, possibly indicating a minor interaction or tidal effects. It would be worthwhile to investigate this galaxy for evidence of weak tidal features, such as faint stellar streams or shells.
