The galaxy presents as a generally smooth, elliptical morphology with a centrally concentrated bulge. It exhibits a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars, consistent with a relatively low rate of on-going star formation. There is little to no evidence of prominent spiral arms or significant dust lanes. The overall shape is moderately elliptical, deviating from a perfect circular form, but is not markedly elongated. No significant tidal disturbances, merging features, or indications of major interactions with other galaxies are readily apparent in this image.
