The galaxy presents as a relatively compact object with a bright central nucleus, suggesting a high concentration of stars and potentially an active galactic nucleus. It appears to have a distorted disk morphology. There is some visual evidence of tidal tails or streams emanating from the main body, indicating possible past or ongoing interaction with another galaxy. The color indices suggest that the galaxy contains both older stellar populations and regions of ongoing star formation. The shape of the galaxy is noticeably elliptical, deviating from a perfect circle. The disk is oriented at a significant angle with respect to our line of sight.
