The galaxy appears to be a relatively compact, elliptical system. Its morphology is generally smooth with a notable absence of spiral arm structures or a well-defined disk. The overall shape is nearly circular, exhibiting a high degree of sphericity. There are hints of minor irregularities, but the primary structure shows no signs of major ongoing mergers or significant tidal disturbances.

The galaxy displays a color gradient, with a redder hue concentrated towards the core region and a slightly bluer color in the outer parts of the galaxy. This color variation suggests differences in stellar populations, with older, redder stars likely dominating the central region and younger, bluer stars possibly present in the outskirts. The limited color contrast could also suggest moderate dust obscuration.
