The galaxy presents as a centrally concentrated object with a relatively smooth morphology. It appears elliptical in shape, exhibiting a high degree of radial symmetry. The light distribution suggests a dominant spheroidal component, possibly an elliptical galaxy or a lenticular galaxy seen face-on. The galaxy has an apparent size of a few arcseconds. Its color profile indicates a population of older stars, which are redder and contribute more to the light in redder bands compared to bluer bands, with an absolute magnitude falling within the range of -21 to -23. There may be some indications of minor disturbances of a merger happening, however the galaxy is mostly stable in its form. The estimated mass is of average size. Star formation is occurring at a low rate.
