The galaxy presents a disk-like morphology, viewed at a moderate inclination relative to our line of sight. There's a discernible central bulge which appears relatively smooth and concentrated. Faint spiral arm features are suggested but ill defined. The disk appears dusty but the overall color is slightly blue shifted towards the bulge, consistent with ongoing star formation. There are no immediately apparent signs of a major recent merger event, although minor irregularities in the disk could indicate past interactions. The galaxy exhibits an overall intermediate luminosity and size.
