The galaxy presents as a relatively compact and luminous object. Its morphology appears largely spheroidal, exhibiting a smooth light distribution with little evidence of spiral arms or a distinct disk structure. The central region is visibly brighter and possibly indicative of an active galactic nucleus or a dense concentration of stars.

The galaxy's color profile suggests it may be composed of an older stellar population, with a noticeable absence of strong blue light, which is typical for galaxies experiencing active star formation. There is no clear evidence of ongoing major mergers or significant tidal disturbances, although subtle asymmetries or minor features cannot be entirely ruled out given the image resolution. The overall impression is that of a passively evolving, massive elliptical galaxy.
