The galaxy exhibits a generally smooth morphology, with a predominantly elliptical shape. It displays a concentrated central bulge with a yellowish hue, suggesting an older stellar population. There is minimal evidence of spiral arms or significant dust lanes. The outer regions of the galaxy appear to fade gradually into the background, lacking a sharp boundary. Overall, the galaxy's light distribution suggests a relatively evolved system with ongoing, but not particularly high, levels of star formation. There is no sign of a major merger and only very slight irregularities in the shape, so there is no indication of a recent minor merger.
