The galaxy presents a predominantly smooth morphology. Its light profile appears centrally concentrated, exhibiting a gradual decline in intensity from the core to the outer regions. The overall shape is largely rounded, with only a slight deviation towards an elliptical form. No distinct spiral arms or bar structures are discernible. There is no obvious evidence of major mergers or tidal disturbances within the immediate vicinity of the galaxy. The color is consistent with that of older stellar populations, likely indicating a relatively low current star formation rate. The galaxy's mass is considerable, potentially indicating a mature system with a long history of star formation.
