The galaxy appears as an elliptical or lenticular type, exhibiting a relatively smooth and centrally concentrated morphology. Its light distribution suggests a high degree of symmetry and a lack of prominent spiral arms or other distinct features typically associated with disk galaxies. There is a slight elongation, deviating from a perfectly circular shape. 

The color profile indicates a predominantly older stellar population, with a notable lack of blue or ultraviolet light, which would be indicative of young, massive stars and active star formation. A slight hint of green color is present, possibly indicative of some older star formation. The overall luminosity is relatively high, suggesting a substantial stellar mass. There is no clear evidence of major ongoing mergers or tidal interactions, although some minor disturbances might be present in the outer regions. 
