The galaxy presents as a slightly elongated structure, displaying an intermediate roundness. It is primarily smooth in appearance, with a notable lack of distinct features such as spiral arms or a prominent central bar. The light distribution within the galaxy appears relatively uniform, suggesting an older stellar population, or a lack of recent major star formation events. There is no evidence of significant ongoing mergers or major disturbances to the galaxy's structure. A slight asymmetry may indicate a minor interaction or internal process subtly affecting its morphology.
