The galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular type. Its shape is elongated, appearing somewhat cigar-shaped, with a gradual increase in light intensity towards the center. The core region exhibits a bright, concentrated luminosity, likely indicative of an older stellar population. Faint blue hues are visible in the outer regions. There appears to be no strong evidence of spiral arm structure, or a central bar. There also seems to be no major galactic merging events occurring. 
