The galaxy presents a largely smooth morphology, with a centrally concentrated bulge dominating its overall appearance. This central region exhibits a yellowish hue, suggestive of an older stellar population. A slight bluer tint is observed in the outer regions, indicating the presence of younger stars or star-forming regions, though these are not clearly resolved. The galaxy appears to be somewhat round in shape. There is no obvious indication of strong tidal features or ongoing major mergers; however, there may be a hint of some minor disturbance.
