The galaxy presents an overall smooth morphology with an elliptical shape. There may be a weak disk component, and appears to be ongoing star formation. The system is not undergoing a major merger, though there might be minor disturbances visible within the galaxy. The galaxy exhibits a moderately high luminosity, placing it among relatively massive galaxies. The colours indicate a mix of stellar populations, with younger, bluer stars likely contributing to the observed star formation activity alongside older, redder stars. The absence of significant dust lanes is also noticeable.