The galaxy presents a generally smooth and rounded morphology, suggesting an elliptical or lenticular type. Its central region exhibits a concentrated, bright yellowish glow, indicative of a dense stellar population. Faint redder emissions are detected, potentially highlighting older stellar populations. There's a slight asymmetry in the light distribution. The overall color is dominated by reddish hues with some green, which may indicate the presence of evolved stars. There is a low likelihood of ongoing major mergers. Minor disturbances may be present.
