The galaxy appears as a centrally concentrated, elliptical-like system. It presents a smooth, largely featureless morphology, with an apparent lack of distinct spiral arms or prominent dust lanes. There is a noticeable radial color gradient, trending from a relatively redder hue in the central region to a bluer tint in the outskirts. This color variation might be due to differing stellar populations, with older, redder stars concentrated towards the galactic center, and younger, bluer stars residing in the outer regions. The galaxy exhibits a moderate degree of roundness in its overall shape, appearing neither highly elongated nor perfectly spherical. There is a hint of a possible minor interaction, or internal disturbance, however there is no prominent major tidal feature visible.
