The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, featureless morphology. It possesses a concentrated, bright central bulge region with a color gradient shifting towards redder hues. The outer regions, while still smooth, appear more diffuse and show subtle color variations hinting at some level of stellar population diversity. There's no clear evidence of spiral arms or significant dust lanes. The galaxy has an overall round appearance with a slight asymmetry, suggesting a possible minor gravitational interaction or past merger event. The spatial extent of the galaxy indicates it is a relatively massive system.
