The galaxy appears as an elliptical-like structure with a smooth light distribution, indicating a lack of prominent spiral arms or distinct features. The central region exhibits a high concentration of light, suggesting a significant bulge component. The galaxy's color profile indicates a predominantly older stellar population, with a gradual shift toward redder hues in the central regions. Faint, diffuse, and slightly bluer light can be observed further away from the center, possibly indicating recent or ongoing star formation. There is some evidence of minor disturbances or asymmetries within the galaxy, which might be attributed to minor interactions. Overall, the galaxy's morphology suggests an older stellar population with the possibility of experiencing some minor gravitational interactions.
