The galaxy presents as a somewhat elliptical structure, suggesting a classification along the lines of an elliptical galaxy, or a lenticular galaxy viewed at an angle. The central bulge is prominent and exhibits a yellowish hue, which indicates a population of older stars. The galaxy's disk, if present, appears relatively smooth, with only subtle hints of spiral arm structure. There is a slight asymmetry to the overall shape, but no significant evidence of ongoing major mergers or tidal disturbances. The color gradient suggests a concentration of older stellar populations in the central region, with a gradual shift towards somewhat bluer, and therefore younger, stellar populations in the outer regions. The galaxy's overall visual smoothness is high, indicative of a well-mixed stellar population and minimal dust obscuration. The morphology leans toward a settled state, possibly nearing the end of its star-forming epoch, although some low-level star formation may still be occurring in the outer regions.
