The galaxy presents as a slightly elongated structure with a smooth, centrally concentrated luminosity profile. It exhibits a color gradient, with the central region appearing bluer, indicative of a younger stellar population or ongoing star formation, surrounded by a more extended, redder halo. The redder halo suggests an older stellar population and possible dust content. The galaxy displays a relatively high degree of smoothness, with no apparent spiral arms or distinct features. There is a slight asymmetry to the morphology, possibly due to tidal interactions or minor mergers with other galaxies. Overall, the galaxy is a relatively faint and compact system.
