The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge and a diffuse halo.  The color profile suggests a mixture of stellar populations, with a yellowish central region possibly indicating older, redder stars, and a slightly bluer outer region indicative of younger, bluer stars. The overall round shape suggests a minimal disk component and no obvious spiral arm structure. There is no apparent evidence of significant tidal disturbances or merging activity.  The light distribution appears even and gradual, diminishing from the core outward. The galaxy appears to be an early-type galaxy with a relatively high degree of symmetry.
