The galaxy presents as a disk galaxy, viewed at an oblique angle. There is an apparent central bulge with a bright, concentrated core. The disk appears relatively smooth, with a subtle color gradient from the central bulge outward, suggesting a decreasing population of older stars. Faint dust lanes are suspected to exist within the disk, with the suggestion of minor disturbances potentially due to a past or ongoing minor merger. The galaxy is estimated to have a considerable stellar mass and a modest rate of star formation. The overall morphology leans towards a smooth appearance with only some indication of internal features.
