The galaxy presents a generally smooth and rounded morphology. There is a central bright region that is diffuse with a fairly high concentration of light. The outer regions of the galaxy gradually fade in intensity and there is not much visible texture. The galaxy is an elliptical type, appearing as a spheroidal mass of stars. Overall, the light profile suggests a relatively evolved stellar population. There are no spiral arm features visible and there is little evidence of ongoing or recent major merging activity. The galaxy appears to be relatively isolated with no signs of significant tidal distortions or disturbances. The color is somewhat uniform throughout, which may imply a fairly homogenous stellar population in terms of age and composition. There are no visible dust lanes or distinct features within the galaxy's disk.
