The galaxy presents as a somewhat elongated structure with a smooth, diffuse appearance. Its central region exhibits a concentration of light, transitioning gradually to a fainter outer region. The color profile appears to be redder in the core, possibly indicating an older stellar population, with hints of green or blue tinges in the outer regions that could suggest the presence of younger stars. There is no strong evidence of distinct spiral arms or a prominent disk. The overall morphology suggests the galaxy could be an elliptical, or possibly a lenticular galaxy seen at an oblique angle. There is no apparent interaction with any other system, but subtle irregularities in the outer regions suggest that there may have been a minor disturbance in its past.
