The galaxy presents as an elliptical or lenticular type. Its morphology appears predominantly smooth, with little evidence of distinct spiral arms or significant dust lanes. The core region exhibits a concentrated, bright luminosity, suggesting a high stellar density, potentially hosting a supermassive black hole at its center.

The galaxy's color gradient transitions from a yellowish-orange core to a bluer, more diffuse outer halo. This color variation may indicate an older stellar population concentrated towards the center, with younger, bluer stars distributed in the outskirts.

There is a subtle hint of asymmetry or a minor disturbance in the outer regions of the galaxy. This could potentially be indicative of a past or ongoing minor merger event with a smaller dwarf galaxy. Overall, it is a relatively isolated galaxy that seems to be in a somewhat evolved state.
