The galaxy presents as a lenticular or possibly early-type spiral galaxy, viewed at a steep inclination. The central bulge appears relatively prominent and ellipsoidal, exhibiting a yellowish-white hue, suggestive of an older stellar population. Faint, diffuse bluish regions extend from the main body, indicating some presence of younger stars and ongoing star formation, though at a subdued rate. The overall structure lacks well-defined spiral arms or distinct features beyond the bulge and a flattened disk component. No evidence of significant tidal interactions or major mergers is discernible. The object's elongated shape indicates the system is not spherical, rather a flattened structure, suggesting a dynamically evolved system where the random motions of stars have decreased, leading to a more ordered structure.
