The galaxy presents as a flattened elliptical or lenticular structure, exhibiting a smooth and relatively featureless morphology. The light distribution is concentrated towards the center, suggesting a significant bulge component. The color gradient indicates a slightly redder hue in the central regions, possibly indicative of an older stellar population, with a subtle transition to bluer tones towards the outer edges. No prominent spiral arms or dust lanes are discernible. The overall appearance suggests a galaxy that has largely completed its star formation. There is no major merger or disruption visible. The object exhibits a moderate degree of roundness.
