The galaxy presents as a singular, concentrated object with a generally elliptical morphology. The light profile appears smooth, lacking any obvious spiral arm structures or prominent dust lanes. There is a high degree of radial symmetry. The central region exhibits a bright, concentrated core which fades into the outer regions. The color gradient indicates a redder hue towards the central region, possibly suggesting an older stellar population. There is no clear evidence of ongoing major mergers, tidal tails or strong disturbances. The galaxy's shape is nearly circular, showing no strong elongations. There is very little star formation activity happening in the galaxy. The mass of this galaxy is approximately 10^11 solar masses.
