The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits a moderate ellipticity, appearing more elongated than perfectly spherical. The color profile suggests a dominant older stellar population, exhibiting a yellowish-red hue, particularly concentrated towards the central bulge. There is little evidence of distinct spiral arm structures or prominent dust lanes. The outer regions appear slightly bluer, possibly indicating the presence of some younger, hotter stars, although star formation activity appears low overall. There are no signs of a major ongoing merger. The galaxy appears to be an intermediate disk galaxy or an elliptical galaxy with a disk-like morphology.
