The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. There is no clear evidence of spiral arms or a distinct disk structure. The color appears to be dominated by redder wavelengths, with a hint of yellow in the central region, suggesting a stellar population that is older or dust obscured. The galaxy does not appear to be undergoing any major mergers or tidal disturbances based on the relatively undisturbed morphology. There is no significant asymmetry in the light distribution. The overall appearance points towards a evolved system, likely an elliptical or lenticular galaxy.
