The galaxy presents as an elongated, spindle-shaped structure. Its light profile appears smooth, with a central concentration of luminosity that fades gradually towards the outer edges. The core region exhibits a yellowish hue, possibly indicating an older stellar population or a higher concentration of dust. Surrounding the core is a fainter, bluish halo, suggesting the presence of a younger stellar population or ongoing star formation activity. There is a slight asymmetry in the outer regions, with one side appearing slightly more extended than the other, possibly a tidal feature or interaction. Overall, the galaxy appears relatively undisturbed, displaying a regular morphology without any prominent spiral arms or irregular features.
