The galaxy presents as a moderately sized elliptical type, exhibiting a high degree of smoothness and roundness. Its color is predominantly yellow-orange, indicating an older stellar population with relatively low ongoing star formation. There is no clear evidence of spiral arms or a prominent disk structure. A slight asymmetry may suggest a past or ongoing minor interaction with another galaxy, however, a major merger seems unlikely due to the overall undisturbed morphology. The galaxy appears to be a fairly massive system, based on its luminosity and size.