The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is little to no discernible spiral arm structure. The color profile indicates a redder hue, suggestive of an older stellar population and a lower rate of current star formation. The overall morphology appears undisturbed, without any obvious signs of tidal interactions or ongoing merger activity. The galaxy exhibits a moderate degree of roundness, leaning towards an elliptical classification rather than a highly flattened disk. The size is relatively compact compared to other galaxies in the field, implying either intrinsic smallness or a significant distance.
