The galaxy presents a spiral morphology, exhibiting discernible arm structures. These arms are primarily composed of tightly wound formations, suggesting a higher density of stellar populations and dust lanes. The arm count appears to be dominated by a single, prominent spiral arm, with possible bifurcations or faint secondary arms emanating from it.

A central bulge region is evident, appearing moderately sized in relation to the overall galactic disk. The bulge displays a concentrated luminosity, hinting at a significant population of older, redder stars. No apparent bar structure bisects the galactic center.

The disk of the galaxy shows evidence of ongoing star formation, apparent due to the blue-ish hue surrounding the center of the galaxy.

There is no immediately obvious presence of a major merger or significant tidal distortions indicative of a recent or ongoing interaction with another galaxy. However, there are minor disturbances present within the system, possibly indicating a mild gravitational perturbation.
