The galaxy appears as a moderately bright, ellipsoidal object. The core is a concentrated region of higher luminosity, exhibiting a yellow-orange hue, suggestive of an older stellar population. The galaxy appears relatively smooth, with no immediately apparent spiral arm structures or prominent dust lanes. The galaxy does not appear to be strongly interacting or tidally disrupted, with no visible distortions or extended features. The overall morphology suggests a possible elliptical galaxy or a lenticular galaxy seen at a relatively low inclination angle, although the resolution limits a definitive classification.
