The galaxy presents a generally smooth, elliptical morphology with a slight elongation. The light distribution is concentrated towards the center, suggesting a prominent bulge. There is a subtle color gradient from a slightly bluer hue in the outer regions to a redder hue near the core. No distinct spiral arms or prominent dust lanes are discernible within the image resolution. There is potentially a minor gravitational disturbance nearby. The galaxy appears to be relatively isolated, with no other galaxies of comparable size in close proximity.
