The galaxy presents as a moderately bright, elliptical-like structure, though it lacks a perfectly smooth appearance. The central region exhibits a high degree of concentration, displaying a yellowish hue suggestive of an older stellar population. There's a slight elongation visible, deviating from a perfectly circular form. Faint disk like structure is visible, but is overwhelmed by a large smooth component. Some blueish knots can be seen near the disk plane indicating ongoing star formation. The galaxy has a reddish component to it at a 45 degree angle from the main structure. Based on the observed color gradients and morphology, this galaxy could be an intermediate mass system with ongoing merger activity.
