The galaxy appears as a single, largely featureless luminous entity. The overall shape is elliptical. A smooth, centrally concentrated luminosity profile is observed with a radial decrease in intensity. The color is generally reddish-yellow, suggestive of an older stellar population, indicative of reduced current star formation activity. There's no clear evidence of spiral arm structures, dust lanes, or distinct nuclei. Faint traces of a more diffuse, slightly bluer halo may be present but are poorly defined. The galaxy appears relatively isolated, showing no obvious signs of recent or ongoing merger events.
