The galaxy presents a smooth, largely featureless morphology, suggesting an elliptical classification or a lenticular galaxy viewed face-on. The object appears centrally concentrated with a smooth falloff in light intensity towards the outer regions, indicating a well-defined spheroidal component. There is minimal evidence of spiral arm structure or dust lanes.

The galaxy exhibits a yellowish-red color, hinting at an older stellar population dominated by evolved stars. The overall color suggests low ongoing star formation. A possible merger could be in the early stages based on the data. The galaxy is moderately large, with an estimated half-light radius of approximately 7 kpc.
