The galaxy presents as a lenticular or edge-on spiral, exhibiting a generally smooth morphology with a high degree of elongation. The central bulge appears bright and yellowish, suggesting an older stellar population. Fainter, bluish light is visible along the outer edges and the disk, potentially indicating some regions of ongoing star formation, albeit at a relatively subdued rate. The overall structure suggests a lack of significant recent merger activity, although subtle irregularities in the disk structure could indicate minor gravitational interactions. The galaxy's orientation provides limited insight into detailed spiral arm structure, if any is present.
