The galaxy presents as a largely featureless, elliptical-like object. It exhibits a smooth, concentrated light profile, suggesting an older stellar population. Its color index indicates a higher concentration of redder wavelengths, consistent with evolved stars and a reduced rate of on-going star formation. There is no indication of spiral arms or a prominent disk structure. The morphology appears relaxed and undisturbed, with no clear evidence of recent merger events. Its overall shape is predominantly round with no obvious tidal features or asymmetric light distribution.
