The galaxy presents as a largely featureless elliptical or lenticular system. The central region exhibits a concentrated, bright yellowish-white core, suggesting an older stellar population. There is a gradual decline in luminosity moving outward from the core. No distinct spiral arms or bar structures are discernible. The shape is primarily rounded, with minimal deviation from circular symmetry. There's no strong visual evidence of ongoing major mergers or tidal disturbances. The galaxy appears relatively isolated and well-defined.
