The galaxy presents a concentrated central bulge, surrounded by a fainter, more diffuse disk. The overall shape appears elongated, with an ellipticity suggesting it is not a face-on spiral galaxy. The light distribution indicates a higher concentration of older stars in the bulge, giving it a reddish hue. There is an apparent disturbance in the surrounding faint halo region, it may suggest some kind of tidal interaction or accretion event. Star formation appears to be present, although not dominant, given the moderate color contrast between the bulge and the disk. The galaxy appears fairly isolated, without any obvious companion galaxies nearby.
