The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light appears to be more yellow-white in the nucleus region, suggesting an older stellar population. The outer regions of the galaxy are fainter and display a slightly bluer hue. There's little evidence of distinct spiral arms or prominent dust lanes, supporting a classification towards the elliptical end of the Hubble sequence. The galaxy shows minimal signs of tidal disturbances or ongoing mergers.
