The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually diffuses into a less defined outer halo. The color profile appears to shift from a yellow-white core to a bluer hue in the outer regions, suggesting a gradient in stellar populations, with older, redder stars likely dominating the core and younger, bluer stars populating the outer regions. The galaxy is somewhat elongated, with a subtle asymmetry in its overall shape; it does not seem to be a perfectly symmetrical ellipse. There is no visible evidence of spiral arms or significant dust lanes. Slight disturbances or minor tidal features might be present in the outer halo, though the image resolution limits definitive assessment. The galaxy seems to be relatively isolated.
