The galaxy presents as a relatively compact, bright elliptical or lenticular system. Its overall color is a yellowish-white, indicating an older stellar population with a likely suppression of recent star formation.

There is a pronounced central bulge that dominates the light profile. This central region appears smooth and symmetrical.

Extending away from the bulge, there is a fainter, elongated structure which may be indicative of a remnant disk component. This structure is characterized by an irregular shape. Within this apparent disk, there appear to be some redder clumps, potentially regions of dust obscuration.

There are no clear signs of spiral arms or active star-forming regions. The system shows a high degree of central concentration with a smooth overall appearance, with signs of a possible past merger event.
