The galaxy appears as a diffuse, moderately luminous object. Its morphology is largely smooth, though subtle features suggest a possible disturbance. The light distribution exhibits an elliptical profile, with the highest intensity concentrated in a central region. A slight elongation is observed, deviating from a perfectly circular shape.

Color gradients are present across the galaxy. The core exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, bluer regions extend outwards from the central region, possibly associated with recent star formation activity in the outer regions. Subtle distortions in the morphology might be attributed to minor gravitational interactions, though no obvious companion galaxies are observed. The overall appearance suggests a galaxy undergoing a relatively quiescent phase, with a moderate level of star formation.
