The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. It exhibits a slight elongation, deviating from a perfectly circular shape. The light is concentrated towards the center, with a gradual decrease in luminosity towards the outer regions. The galaxy exhibits a yellow-red hue across its entirety, hinting at an older stellar population, and a lack of significant recent star formation. There is some visual evidence of a possible minor disturbance or interaction occurring with what appears to be another galaxy, evidenced by a potential tidal tail or distorted shape.
