The galaxy presents as a centrally concentrated object with a relatively smooth, diffuse appearance. There is a subtle elongation, but it appears mostly round. The light distribution suggests a centrally dominant bulge component. A faint blueish tint to the galaxy's overall color indicates the presence of some young, hot stars and recent star formation, although the smooth morphology suggests that star formation is not happening at a very high rate. There is no apparent spiral structure or bar visible. There is no noticeable dust lane obscuring the galaxy's light. The overall impression is that of a mature galaxy, potentially in the transition between a spiral and elliptical morphology. It does not appear to be undergoing any major mergers or tidal interactions with other galaxies.
