The galaxy presents a morphology consistent with an elliptical galaxy, exhibiting a predominantly smooth light distribution. There appears to be little to no indication of significant spiral arm structure or a prominent disk. The overall color suggests an older stellar population with a bias toward redder wavelengths, which is typically associated with galaxies with less active star formation. The galaxy is approximately round in shape with some signs of slight elongation. The absence of strong tidal features or signs of ongoing mergers suggests the galaxy has likely undergone a relatively quiescent evolutionary history recently.
