This galaxy presents as a flattened, elliptical structure. The central region exhibits a pronounced bulge, appearing smooth and concentrated with a yellowish-orange hue, indicative of an older stellar population. Extending outward from the bulge, the galactic disk displays a gradual decrease in luminosity. There are faint hints of bluer regions within the disk on opposite sides of the bulge, suggesting possible regions of more recent star formation. The galaxy's overall morphology suggests it has undergone some evolutionary processes, possibly merging or tidal disruption with other galaxies. There does not appear to be evidence of spiral arms, nor any significant dust lanes visible in this image. The galaxy's elongated shape suggests it may be a lenticular galaxy.