The galaxy presents a relatively compact, centrally concentrated appearance. Its morphology is not clearly defined, lacking a prominent spiral structure or elliptical form. The central region exhibits a bright, almost stellar-like core, surrounded by a diffuse, less luminous halo. The halo displays an irregular shape, suggestive of potential tidal interactions or ongoing merging activity. The color distribution shows a central concentration of bluer wavelengths, potentially indicating recent or ongoing star formation, with the outer regions appearing redder, possibly indicating an older stellar population. Faint, wispy extensions are observed on one side of the galaxy.
