The galaxy presents as a somewhat elliptical structure with a prominent central bulge. The light from the bulge appears yellowish. The disk component is less defined, exhibiting a smoother, more diffuse appearance. The colors become slightly bluer toward the outer edges, suggesting the presence of a younger stellar population in these regions. No distinct spiral arms or bar structures are readily apparent. There might be a subtle indication of minor tidal disturbance or faint asymmetry in the galaxy's outer halo, but this is not definitively discernible from the image alone. The galaxy appears relatively isolated, with no obvious signs of interaction with nearby galaxies.
