The galaxy presents as a relatively smooth elliptical form. The central region exhibits a bright, concentrated core that gradually diffuses outwards. The overall color appears to be a pale blue/white, suggestive of an older stellar population with perhaps ongoing, albeit low, levels of star formation. The shape is elongated. There is no discernible spiral structure. The edges of the galaxy fade gradually into the background, lacking any sharp boundaries or tidal features. No evidence of a recent major merger is apparent, though the slight elongation may be indicative of a minor interaction in the past.
