This galaxy presents an elongated, cigar-shaped morphology. A bright, concentrated central bulge is visible, surrounded by a less defined and dimmer disk. The light distribution in the disk appears relatively smooth, with some clumpy regions. There is evidence of disturbance or asymmetry in the galactic structure, possibly indicating a minor interaction or merger event.

The color gradients suggest a slightly bluer population in the disk, compared to the redder central bulge. This could indicate ongoing star formation in the disk. The galaxy appears to be at a considerable distance, with an estimated size of approximately 6 kpc across its major axis. The overall features align more with those of a late-type spiral galaxy rather than an elliptical galaxy, suggesting the presence of spiral arms, which are not very distinct from this view.
