The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge that graduates outwards into a less dense halo. The overall shape deviates slightly from a perfect circle, exhibiting a mild elongation. Color gradients are discernible, with the central bulge appearing yellowish, possibly indicating an older stellar population, while the outer regions show a hint of bluer hues, suggesting the presence of younger stars. There is no distinct indication of spiral arm structures or significant dust lanes. The galaxy does not appear to be undergoing any major merging activity or showing signs of significant tidal disruption. The general morphology suggests that the galaxy is a disk-like object seen at an angle.
