The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. The light distribution suggests a relatively old stellar population, indicated by the redder hues emanating from the core region. There is some indication of possible tidal disturbances or faint plume-like structures extending from the main body, suggesting that the galaxy may be undergoing or have recently undergone a merger event, though the evidence is not conclusive. The overall shape deviates somewhat from a perfect ellipse, exhibiting a slight irregularity. The galaxy has an estimated size of approximately 7.5 kpc. It exhibits moderate levels of star formation.
