The galaxy presents as an elliptical morphology, appearing mostly smooth with a concentrated central bulge. It exhibits a predominantly yellow-orange color, suggesting a population of older stars and a lower rate of ongoing star formation. The light distribution appears relatively symmetrical, with a high degree of roundness. There is no visible evidence of spiral arms or a prominent disk structure. The object appears isolated, showing no clear signs of major merger activity or significant tidal disturbances. However, there is a slight asymmetry, indicating a possibility of minor gravitational interaction. Based on the color and morphology, this galaxy is likely a massive elliptical with a significant population of evolved stars.
