The galaxy exhibits a generally smooth morphology, with a slight elongation. The color profile suggests a dominant population of older stars, with a bluer core possibly indicating a region of more recent, though not exceptionally vigorous, star formation. The galaxy displays some evidence of a disturbance, possibly indicating an ongoing or recent interaction with another galaxy. There is no clearly defined spiral structure or a prominent central bulge, which suggests that this galaxy is likely an elliptical or lenticular type.
