The galaxy presents a generally smooth appearance, exhibiting a morphology indicative of an elliptical or lenticular type. There's a centrally concentrated bulge that dominates the overall luminosity. The galaxy appears more or less rounded. There might be minor disturbances or interactions influencing its morphology, but there is nothing major. The galaxy exhibits a color gradient, transitioning from yellowish hues in the central bulge to slightly bluer tones in the outer regions, suggesting the presence of some ongoing star formation. The galaxy spans approximately 6 kiloparsecs in diameter. The estimated mass indicates a substantial system. Overall, this galaxy appears to be a massive elliptical or lenticular galaxy with evidence of moderate star formation activity.
