The galaxy presents as an elongated, spindle-shaped structure. It displays a smooth, largely featureless morphology. The central region exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Progressing outwards from the core, the color transitions to a bluer shade. This might suggest some on-going or recent star formation on the outskirts, or the presence of a more diffuse distribution of younger, bluer stars within the galaxy’s halo. The object appears relatively isolated, with no obvious signs of major tidal distortions or interactions with other galaxies in its immediate vicinity. Subtle irregularities in the outer regions may indicate a minor disturbance, but the overall structure points towards a settled state.
