The galaxy presents as an elongated, cigar-shaped structure, strongly suggesting an elliptical morphology viewed at an oblique angle. The central region exhibits a high surface brightness, appearing bright yellow, indicative of an older stellar population. The outer regions display a gradual decline in surface brightness, with a faint, diffuse halo surrounding the central bulge. There's a subtle color gradient from the center outwards, possibly due to a shift in stellar populations. There is no obvious evidence of spiral arm structure or active star formation regions. Overall, the galaxy appears to be a relatively undisturbed system, lacking any significant signs of recent mergers or tidal interactions.
