The galaxy presents as a somewhat elliptical, though largely spheroidal, object with a concentrated central bulge. There is a noticeable color gradient, transitioning from a yellowish-white core to a bluer, fainter periphery.  While no distinct spiral arm structures are visible, there appears to be a very faint disk component. The galaxy's overall structure appears largely undisturbed, with no apparent signs of major mergers or significant tidal disruptions. The galaxy's light profile is smooth, suggesting a relatively old stellar population dominating the overall light output, although the bluer periphery hints at some ongoing star formation.
