The galaxy presents as a largely spheroidal system, appearing smooth and relatively featureless in the available imagery. There is a bright, concentrated central region, possibly indicative of a substantial bulge component. The galaxy exhibits a noticeable radial color gradient, transitioning from a yellowish-white core to a redder halo. This may suggest an aging stellar population in the outer regions. The overall morphology suggests that the galaxy is likely an elliptical or S0 type. There is no immediately apparent evidence of ongoing major mergers or significant tidal disturbances. There's a slight hint of a very faint disk.
