The galaxy presents an elongated, disk-like morphology, suggestive of a spiral or lenticular galaxy viewed edge-on. The central region exhibits a brighter, concentrated luminosity profile, possibly indicating a bulge. A relatively smooth texture across the galactic disk is observed, with some hints of dust lanes or spiral arm structures, although these are not distinctly resolved. The color distribution is somewhat uneven, displaying a central bluish hue, which may correspond to recent star formation activity. The outer regions of the disk appear fainter, and their color seems to shift toward a redder spectrum, possibly due to an older stellar population. The galaxy appears relatively isolated. No clear signs of strong tidal interactions or mergers are evident in the immediate vicinity, though subtle features might be present.