The galaxy appears as an elliptical or spheroidal structure, exhibiting a smooth, relatively featureless morphology. The central region displays a concentrated brightness, suggestive of a significant stellar population. The light profile gradually decreases with radial distance from the core, indicative of a centrally-peaked stellar distribution. The galaxy exhibits a predominantly yellow-red hue. Overall, the galaxy presents itself as a mature system with minimal discernible signs of ongoing major star formation or disruptive interactions. A slight elongation is observed, hinting that the galaxy may not be perfectly spherical. There is a very slight hint of a disc, although this is far from clear. Based on its smooth morphology and redder colours, I estimate the galaxy to be fairly massive.
