This galaxy presents as an elongated, disk-like structure, displaying a significant degree of ellipticity. The central region exhibits a concentrated, bright core suggesting a prominent bulge. Moving outwards from the core, the luminosity gradually decreases, transitioning into a fainter, more diffuse disk. This disk component appears relatively smooth, with little evidence of distinct spiral arm structures.

The colour profile indicates a range of stellar populations. The core and inner regions exhibit a yellowish-white hue, suggestive of older, more evolved stars. The outer regions of the disk display a bluer tint, potentially indicating the presence of younger, hotter stars and ongoing star formation.

Based on the morphology, it is likely a spiral galaxy seen edge-on or a lenticular galaxy. There is no evidence of strong tidal interactions or major mergers, but minor disturbances cannot be ruled out based on the image alone.
