The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. It has a generally rounded morphology. There is no strong evidence of a prominent disk structure or spiral arms. Minor disturbances may exist based on slight asymmetries, but it does not seem to be undergoing a major merger or interaction with another galaxy. The galaxy's color profile suggests an older stellar population, biased towards the redder end of the spectrum, with a moderate amount of ongoing star formation. The galaxy is relatively compact, with a moderate size.
