The galaxy presents as a spiral type, exhibiting a clear disk structure. The spiral arms are well-defined, showcasing a distinct winding pattern originating from the central bulge. These arms display variations in brightness and color, suggestive of differing stellar populations and ongoing star formation regions.

The central bulge appears moderately sized, possessing a yellowish hue indicative of an older, more evolved stellar population. A bar structure seems to be present within the central region, though it's not exceptionally prominent.

There's evidence of some disruption or interaction, possibly a minor disturbance, as the spiral arms show some degree of asymmetry or warping. Overall, the galaxy appears relatively undisturbed, with a morphology primarily driven by internal dynamics rather than significant external interactions. The estimated size suggests it is a typical spiral galaxy, neither exceptionally large nor particularly small.
