The galaxy presents an elongated, cigar-like shape, suggesting an elliptical morphology. A smooth central bulge is visible, exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions appear fainter and possess a bluish tint, hinting at the presence of younger, hotter stars and ongoing star formation activity. There is no clear evidence of spiral arms or a well-defined disk structure. The overall appearance suggests the galaxy is relatively undisturbed, without signs of recent major mergers, though subtle asymmetries or minor disturbances cannot be entirely ruled out.
