The galaxy appears to be a relatively smooth, elliptical-like structure. The central bulge exhibits a more concentrated, bright orange-ish hue, suggesting an older stellar population. Progressing outwards from the center, the galactic disk displays a gradual decline in orange color. The outskirts of the galaxy show a much fainter greenish-blue tone, hinting at a small population of younger, hotter stars, and possibly some ongoing, but very limited star formation. There is little evidence of spiral arm structure or significant dust lanes. The overall morphology suggests a fairly evolved system with a dominant spheroidal component. It is highly round in shape, although the distribution of bluer light hints at a disk. No obvious signs of major merger activity or tidal disturbances are present.
