The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. A slight elongation is visible, transitioning from a bright, concentrated central region towards a fainter, more diffuse outer halo. There is a general lack of distinct spiral arm structures or prominent dust lanes.

Color gradients suggest an aging stellar population; the central bulge exhibits a yellowish hue, potentially resulting from older, redder stars, whereas the outer regions display a faint bluish tint.

The overall structure suggests a relatively evolved system, with a high degree of internal order and a well-established gravitational equilibrium. No strong tidal features or indications of recent major merger events are immediately apparent.
