The galaxy presents as a slightly inclined spiral. Its morphology is characterized by a central bulge region exhibiting a moderate concentration of light, with a substantial portion of the galaxy's luminosity emanating from the disk. Evidence suggests the presence of spiral arms, although their structure appears somewhat flocculent and disrupted, with considerable patchiness in stellar distribution and star-forming regions.

Based on the image, the galaxy exhibits a blue hue, indicating a population of young, hot stars. The degree of disturbance suggests possible ongoing or recent interactions. There is no obvious central bar structure. A low amount of dust is assumed.
