The galaxy presents an overall elliptical morphology, appearing as a flattened spheroid. A prominent central bulge is evident, exhibiting a high concentration of light. Fainter, more diffuse regions extend outwards from the bulge, with the major axis oriented at approximately 45 degrees relative to the horizontal. The galaxy appears bluish in color, suggesting the presence of a relatively young stellar population and active star formation. Hints of spiral structure, though not sharply defined, may be present in the outer regions. There is little evidence of significant dust lanes or strong tidal features, although the disk appears slightly disturbed in the image. 
