The galaxy appears as an elliptical or lenticular system, presenting a generally smooth and rounded morphology. There is a primary, concentrated bulge of older stars dominating the central region, exhibiting a yellowish-orange hue suggesting an older stellar population and lower levels of ongoing star formation.

A very slight asymmetry is present, with a possible small companion or tidal feature detectable to one side. This could indicate a past or ongoing minor interaction or merger event. There are no prominent spiral arms visible. The overall color gradient suggests a central concentration of evolved stars with potentially diminishing star formation activity towards the outer regions. The galaxy is relatively compact and appears undisturbed, maintaining a high degree of sphericity.
