The galaxy presents as a generally smooth object with a somewhat elongated, elliptical morphology. The central bulge exhibits a high surface brightness, appearing bright and concentrated with a yellowish hue. Progressing outwards from the core, the galaxy gradually fades into a fainter halo. There is a subtle asymmetry, with one side appearing slightly more extended than the other. No distinct spiral arm structures or significant dust lanes are apparent, suggesting a classification towards the early-type end of the Hubble sequence. There appears to be some disturbance or interaction occuring.
