The galaxy appears as a centrally concentrated object with a smooth overall morphology. The light distribution suggests a dominant spheroidal component. There is a notable absence of spiral arm structures or prominent dust lanes, which is consistent with an elliptical or lenticular galaxy classification. The galaxy's color is predominantly yellowish-orange, indicating a stellar population dominated by older, redder stars, with little evidence of active star formation regions. The galaxy exhibits a relatively high degree of roundness in its overall shape, and there does not appear to be evidence of any major tidal disturbances or ongoing merger events.
