The galaxy presents as an elliptical morphology, appearing elongated with a cigar-like shape. Its light distribution is relatively smooth and concentrated towards the center, exhibiting a central bulge that gradually fades into the outer regions. The overall color is a yellowish-white, suggestive of an older stellar population with fewer young, hot, blue stars. There is no apparent dust lane or spiral arm structure visible, and there is no evidence of any significant ongoing merging activity or major disturbances in the galaxy's structure.
