The galaxy appears to be an elliptical type, exhibiting a generally smooth and centrally concentrated morphology. There is a bright, prominent central bulge, which decreases gradually in luminosity outward. The overall shape approximates a slightly rounded ellipse. Faint, diffuse extensions are noted along what appears to be the major axis, indicating a possible disk component. There is a suggestion of some disturbance to the disk, or arm-like structures, in the periphery, but it is difficult to resolve. No major signs of ongoing merging activity are apparent, however, the slight disturbances might point to a past minor merger event. The galaxy demonstrates colors trending towards the red end of the spectrum, suggesting an older stellar population is dominant.
