The galaxy presents as a spiral galaxy, viewed at a significant angle relative to its face-on orientation. The central bulge appears small and somewhat indistinct, indicative of a possibly less massive bulge component. The galactic disk displays a degree of irregularity, possibly suggestive of interactions or mergers, with a noticeable warping along its length. The arms are not clearly defined, but seem patchy and diffuse, with a somewhat clumpy distribution of star-forming regions. The disk shows variations in colour, consistent with the presence of both younger, bluer stellar populations and older, redder populations. There may be a sign of disruption in the morphology that suggests a possible merger event in its past.
