The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. There is no discernible spiral arm structure or prominent dust lanes. The color profile suggests an older stellar population, dominated by redder wavelengths with only a slight contribution from bluer wavelengths, indicative of ongoing, albeit subdued, star formation. The overall shape appears largely spheroidal, with minimal visible distortions or signs of recent major mergers. The galaxy is moderately luminous, and likely a significant mass. Faint, diffuse light extends outwards from the core, fading gradually into the background sky.
