The observed galaxy presents a spiral structure, viewed at an angle somewhat between face-on and inclined. Tightly wound, defined spiral arms emanate from the central region, exhibiting a blue hue suggestive of ongoing star formation. There is some evidence of faint, extended spiral arms reaching further out into the galaxy's disk.

The galaxy possesses a prominent bulge, approximately a quarter of the galaxy's overall size, which presents a yellow-orange color indicative of an older stellar population. The central bulge appears relatively smooth, suggesting a lack of significant dust obscuration in that region.

Disturbances and tidal tails cannot be clearly identified in the visible structures. The galaxy's overall morphology suggests it is not currently undergoing a major merger. There is no strong evidence of a prominent bar structure.
