The galaxy presents as a concentrated, centrally dominant structure with a smooth morphology. It appears relatively round, with a slight deviation towards an intermediate ellipticity. There is no clear evidence of distinct spiral arms or a prominent disk. It exhibits a yellow-white hue, suggestive of a stellar population dominated by older stars. No strong tidal features or signs of ongoing mergers are immediately apparent, although a minor disturbance cannot be ruled out. The galaxy's light is concentrated and diffuse, indicative of a substantial mass. The overall appearance suggests a relatively quiescent galaxy, potentially an elliptical or S0 type, with a moderate level of star formation.