The galaxy presents as a largely smooth, elliptical-like structure. It appears to be dominated by an older stellar population, judging by the yellowish-red hue of the central bulge. The light is centrally concentrated, with a gradual fading toward the edges. There's little evidence of strong spiral arm structures or significant dust lanes from this vantage point. A slight asymmetry or minor disturbance appears in the outer regions, specifically at the top, where a very subtle and elongated feature exists. Otherwise, the galaxy exhibits a generally well-defined and rounded morphology, lacking any indications of a major ongoing merger.
