The galaxy presents as a generally smooth object with a concentrated central bulge. The morphology appears to be elliptical, with a moderate degree of ellipticity. The color profile indicates a redder hue toward the outskirts and a comparatively bluer tint within the core region, suggesting a difference in stellar populations and star formation activity within those two regions. The galaxy appears to be fairly isolated with no apparent tidal tails or strong morphological distortions indicative of recent major merger activity, although there is a possibility of minor disturbances given the slight asymmetry in the outer regions. Overall, it is consistent with a relaxed galaxy having a largely quiescent star formation history.
