The galaxy presents as a moderately luminous, centrally concentrated object. It exhibits a somewhat amorphous structure, lacking sharply defined spiral arms or a prominent bar. The core region appears yellowish-white, potentially indicating an older stellar population and lower star formation rate. Surrounding the core is a more diffuse, bluish halo. This suggests the presence of a younger stellar population contributing to the overall blue light. The galaxy’s morphology is tending more towards smooth rather than possessing a disk. The observed shape is somewhat in between a perfectly round or cigar shape. There does not appear to be a signs of major mergers occurring with other galaxies.