The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that appears mostly spheroidal with diminishing light intensity towards the outer edges. The galaxy's overall color is slightly redder with a tinge of blue in the outskirts, indicating the presence of both older stellar populations in the bulge and some younger, star-forming regions within its disk. There seems to be a slight disturbance in the galaxy that hints at a possible tidal interaction or minor merger event. No distinct spiral arm structure is clearly visible, but the galaxy does have a disk-like component. The galaxy presents an overall rounded morphology, with deviations from perfect circularity.
