The galaxy presents as a relatively smooth, centrally concentrated object. It appears somewhat elliptical in shape, with a subtle elongation rather than a distinct disk structure. The central region exhibits a bright, concentrated core, possibly indicating an active galactic nucleus or a dense stellar population. The galaxy's color profile suggests a predominantly older stellar population, with a general lack of significant blue star formation regions. There may be some minor disturbances in its form, although the galaxy appears to be in a generally relaxed state with no major ongoing mergers.
