The galaxy appears to be an elliptical type. It has a generally smooth morphology, with a concentrated central bulge that exhibits a yellow-orange hue, suggesting an older stellar population. The galaxy's profile is moderately elongated. There is some indication of a faint, diffuse disk surrounding the central bulge, showing subtle blueish tones. This disk structure is not prominent, it seems like a faint structure surrounding the bulge. There are no clear signs of spiral arms or ongoing major mergers within the galaxy, however, there might be very subtle tidal disturbance in the halo. Overall, the galaxy seems fairly evolved.
