The galaxy presents as a singular, moderately luminous object with a smooth, largely featureless morphology. Its shape is consistent with a spheroidal classification, appearing almost perfectly round. There is a subtle color gradient visible, with the central region exhibiting a slightly more yellow hue, potentially indicative of an older stellar population. No distinct spiral arms, bars, or dust lanes are discernible. The overall impression is that of a relatively undisturbed galaxy, not currently undergoing any major merger events or experiencing significant star formation activity. The faintness and lack of distinct features are likely due to its considerable distance.
