The galaxy presents as a singular, well-defined object with an elliptical morphology. A smooth light distribution dominates, suggesting a largely featureless structure, without evidence of spiral arms or significant dust lanes. The galaxy exhibits a concentrated central bulge that gradually fades into the outer regions. The color gradient transitions from a yellowish-white core to a subtly redder halo, possibly indicating a varied stellar population with older, redder stars dominating the periphery. There is no clear evidence of tidal disturbances or ongoing mergers with other galaxies, indicating it is likely an evolved, relatively undisturbed system. The size appears moderate, suggesting a galaxy of substantial, but not exceptionally large, physical extent.
