The galaxy presents as a relatively compact object. Its morphology appears generally elliptical, with a somewhat amorphous halo surrounding a brighter, more concentrated central region. The color profile is dominated by yellow-red hues, particularly in the core, with subtle blue tinges in the outer regions, suggesting the presence of younger stellar populations, though the older, redder populations appear to be dominant. There appears to be a slight asymmetry in the distribution of the bluer regions, with a more pronounced concentration on one side of the galaxy, indicating a potential disk feature. Overall, the galaxy seems to be in a relatively evolved state with ongoing, but possibly low-level, star formation. There is no clear evidence of spiral arm structure or strong tidal disturbances.
