The observed galaxy presents as a spiral galaxy, viewed at a significant angle relative to its disk plane, though not entirely edge-on. The spiral arms are prominent and well-defined, exhibiting a clumpy, heterogeneous structure indicative of star-forming regions. A central bulge is present, although not particularly dominant, suggesting a relatively late-type spiral classification. The bulge appears yellowish-white in color. The disk shows a mottled bluish hue, characteristic of younger stellar populations. There is evidence of a bar structure within the central region, which could be moderately weak or a strong. No signs of significant tidal disturbances are observed. Overall, the galaxy appears relatively undisturbed, showing no signs of recent major mergers or interactions.
