The galaxy exhibits a predominantly smooth morphology, suggesting it is likely an elliptical or lenticular type. Its overall shape is generally round. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy appears to be dominated by an older stellar population, indicated by its reddish-yellow color. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions. There is no apparent ongoing major merger activity, although some minor disturbances or tidal features cannot be ruled out based on this image alone. Overall, the galaxy appears to be a relatively quiescent system with a low rate of star formation.
