The galaxy appears to be a relatively smooth, elliptical-like structure. It presents an elongated morphology, exhibiting a cigar-like shape rather than a perfectly round appearance. There is no apparent presence of a distinct disk or spiral arms. The galaxy's light is concentrated towards the center, indicative of a dense galactic nucleus. The overall color profile suggests a stellar population that is not dominated by young, blue stars, but more of an older redder population. There are no signs of significant recent or ongoing merging activity or major disturbances in the galaxy's structure.
