The galaxy presents as a roughly elliptical, albeit somewhat irregular, form. The core exhibits a yellowish hue, suggesting a population of older stars. Moving outwards, a gradual shift towards bluer tones is observed, indicative of more recent star formation. The galaxy does not display well-defined spiral arms, yet there seems to be a disk feature. Patches of reddish color are visible, potentially highlighting areas with dust obscuration or regions of ionized gas. The galaxy's overall structure appears relatively smooth, although there may be minor disturbances. Faint extensions or tidal features cannot be ruled out with the available image resolution, suggesting there is some interaction happening. The galaxy does not exhibit a pronounced central bulge.
