The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. The galaxy appears to be generally intermediate in roundness, being neither perfectly circular nor extremely elongated, tending more towards elliptical than disk. The presence of distinct spiral arms or a well-defined disk structure is not apparent. There is no strong evidence of ongoing mergers or major tidal disturbances, though some minor irregularities are noted in the galaxy's outer regions. Color gradients suggest a higher concentration of older stellar populations in the central bulge, with slightly bluer hues in the surrounding regions possibly indicating pockets of more recent star formation. The overall color index suggests the galaxy is a relatively red and potentially quiescent system.

