The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be largely featureless, lacking prominent spiral arms or a distinct bar structure. The galaxy exhibits a generally elliptical morphology, appearing moderately rounded. There is a suggestion of minor disturbances in the galaxy's overall structure. The color profile indicates a tendency towards bluer light in the central regions, transitioning to slightly redder hues in the outer parts. This may reflect on-going star formation activity.
