The galaxy appears to be a relatively smooth, elliptical galaxy, presenting a fairly uniform luminosity profile. It appears circular in shape, indicating we may be viewing it close to face-on. There is no clear evidence of a spiral structure or a prominent disk. The galaxy is characterized by a central, somewhat brighter region, suggesting a possible concentration of stars or an active galactic nucleus. Color indices suggest the presence of older stellar populations. There is no obvious ongoing major merger activity or significant tidal disturbances in this image.
