This galaxy appears to be an elliptical galaxy exhibiting a smooth morphology. Its overall shape is elongated, but not strongly so, leaning more towards a slightly flattened spheroidal structure. The color gradient suggests a centrally concentrated stellar population, with the core exhibiting a yellowish-orange hue. This core likely consists of older, redder stars. The outer regions of the galaxy show hints of a bluer population, which could indicate the presence of younger stars or ongoing, albeit low-level, star formation in the outer disk. No prominent dust lanes or spiral arms are visible. There seems to be no significant sign of tidal disturbances or ongoing mergers from the overall shape. The galaxy appears mostly undisturbed.
