The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a radial decrease in surface brightness. There is a slight asymmetry to the galactic halo, with a very faint suggestion of tidal disturbances. The color profile suggests an older stellar population dominating, indicated by the redder hue. There is some marginal indication of residual star formation within the galaxy, however the overall rate appears low. The morphology is roughly spherical in shape. There are no visible spiral arms, bar structures, or dust lanes. It appears to be in a relatively isolated environment.
