The galaxy presents with an elliptical morphology, displaying a somewhat elongated shape with a slight offset or irregularity in its form. The galaxy is neither perfectly round, nor does it possess a highly flattened, disk-like structure. The central region of the galaxy exhibits a brighter, concentrated core suggesting a higher density of stars. There appears to be a possible tidal tail or distorted feature extending from the main galactic body on one side, which could be indicative of a previous or ongoing interaction with another galaxy.

The galaxy exhibits a subtle color gradient, with a central bluish hue possibly indicating regions of more recent star formation. The outer regions appear somewhat redder, which may suggest an older stellar population. Based on the observed features, this galaxy shows evidence of being an intermediate mass galaxy with some signs of possible recent or ongoing interaction influencing its morphology and star formation properties.
