The galaxy presents as an elongated, disk-shaped structure with a relatively smooth and featureless appearance at this resolution. The central region exhibits a higher surface brightness, indicating a concentration of stars toward the galactic nucleus or bulge. The color appears to be predominantly yellow-orange, suggesting an older stellar population dominates the light output. The disk of the galaxy appears tilted relative to the observer's line of sight. While no distinct spiral arms are visible, there is a subtle hint of structural irregularity suggesting a possible barred spiral morphology. There is no clear evidence of active galactic nuclei or intense star formation regions, such as bright HII regions or dust lanes. The galaxy appears fairly isolated. It is difficult to estimate the exact morphological type, but it appears to be an early type spiral or a lenticular galaxy.