The galaxy presents as an elliptical or lenticular morphology, exhibiting a generally smooth and centrally concentrated light distribution. There is evidence of a bulge, with a noticeable decrease in luminosity moving outward from the galactic center. The overall color appears to be composed of a mix of redder and bluer hues, which may indicate a range of stellar populations. It's overall disk-like in shape, but there are not obvious spiral arms or features that stand out as particularly bright regions of star formation. There's no obvious sign of galactic tidal tails or other obvious structures. The galaxy is generally undisturbed.
