The galaxy presents a smooth, elongated morphology, appearing cigar-shaped when viewed from our perspective. The light distribution is relatively uniform, lacking a pronounced central bulge or spiral arm structure. Color gradients are subtle, exhibiting a central region with a yellowish hue that fades to a bluer tint at the galaxy's edges. The lack of distinct features suggests a relatively evolved stellar population, although some ongoing star formation cannot be ruled out based on the bluer color at the edges. There are no obvious signs of a major merger or significant tidal disturbance. Overall, this galaxy appears to be a relatively undisturbed, elongated system with a mix of older and younger stellar populations.
