This galaxy presents as an elliptical or lenticular system, exhibiting a smooth, diffuse light distribution with a high degree of central concentration. The overall color appears reddish-yellow, suggesting an older stellar population with a lower proportion of young, massive stars. The galaxy's shape is moderately elongated, deviating slightly from perfect circularity. There is a suggestion of a minor disturbance or interaction in the form of an adjacent, redder, and somewhat amorphous light concentration on the periphery of the main galaxy, perhaps indicating a minor merger event or tidal interaction. There is no clearly discernible spiral arm structure. The overall morphology suggests a relatively passive system with a suppressed star formation rate.
