The galaxy appears to be a relatively smooth, elliptical-like structure. The light is concentrated towards the center, showing a bright central bulge or core. The galaxy has a generally rounded morphology and exhibits a color gradient transitioning from a slightly bluer hue in the outer regions to a redder color near the core, suggesting an older stellar population concentrated towards the center. No prominent spiral arms or significant dust lanes are readily apparent. It appears that there is little or no ongoing major star formation, but the blue colors in the outer regions suggests there is some star formation occurring. The galaxy does not show any signs of major tidal disturbances or ongoing mergers.
