The galaxy presents as a moderately luminous elliptical galaxy, exhibiting a smooth, relatively featureless morphology. Its overall shape is generally round. The central region displays a high concentration of light, decreasing gradually towards the outer edges. The color profile indicates a redder hue, suggesting an older stellar population and potentially a lower rate of current star formation activity. There is no obvious indication of a spiral structure or ongoing major merger events. Minor asymmetry is suspected. The galaxy appears to be relatively isolated.
