The galaxy presents as a concentrated, elliptical-like structure with a smooth, featureless appearance. The central region exhibits a bright, yellowish-white luminosity that gradually diffuses towards the outer edges. No distinct spiral arms or bar structures are discernible. The overall color profile suggests a population dominated by older stars, potentially indicating a relatively quiescent star formation history. The lack of defined features could be indicative of a more dynamically relaxed system. The edges are not well defined, they gradually fade into the background sky. There are signs of possible galactic merging with minor disturbances that can be seen in the image.